The galaxy presents a diffuse, somewhat amorphous morphology. The central region exhibits a bright, concentrated luminosity, suggesting a prominent galactic nucleus. The overall shape appears neither perfectly spherical nor distinctly disk-like, tending more towards an elliptical form, though with some irregularity. 

Coloration is generally consistent, with a slightly redder hue concentrated in the central bulge, potentially indicating an older stellar population. Fainter, bluer components are tentatively discernible in the outer regions, suggesting the presence of younger stars or ongoing star formation, albeit at a low level. Indications of tidal disturbances, minor distortions, or interactions with other galaxies are not clearly evident but not entirely absent. There are suggestions of faint arms or plumes extending from the central region, though definitive classification is hampered by the galaxy's diffuse nature. The galaxy does not seem to show any indication of a major merger, but may have experienced a minor one at some point.
