The galaxy presents as an elongated structure, exhibiting a relatively smooth morphology. The central region appears brighter and more concentrated, suggesting a prominent galactic bulge. Moving outwards from the center, the light distribution gradually fades towards the edges of the galaxy, indicative of a diffuse outer disk or halo. The overall color profile suggests a mix of stellar populations, with some bluer regions possibly indicating ongoing star formation, while the redder hues may represent older, more evolved stars. There is slight asymmetry in the distribution of light, suggesting possible gravitational interactions or past merger events. There is a slight hint of a disk structure, but it is not well defined. The image resolution does not permit a detailed examination of spiral arms or other fine-scale features.
