The galaxy presents as a moderately sized, complex structure. Its overall shape is somewhat elliptical, exhibiting characteristics that fall between a distinctly round and an elongated morphology. The light distribution suggests a partially smooth profile, yet with noticeable features indicative of internal structure or ongoing interactions.

A dominant feature is a central, brighter region, potentially indicating a concentrated nucleus or bulge. Extending from this central region are less defined, diffuse arms or extensions. The color gradients within the galaxy are noticeable. A shift towards slightly redder hues is evident within the core, transitioning to bluer tones in the more extended regions. These color variations suggest differential stellar populations or dust content across the galaxy's structure.

Indications of disturbances or tidal features can be discerned, suggesting potential merger events or gravitational interactions with other galaxies. These appear as asymmetries or distortions in the outer regions of the galaxy. Dust lanes or obscured regions may be present, contributing to the patchy appearance in certain areas. High-resolution imaging and spectroscopic analysis would aid in confirming these features and characterizing the galaxy's evolutionary state.
