The galaxy presents a moderately inclined, disk-like morphology. It exhibits a central bulge that appears relatively bright and somewhat diffused, suggesting an older stellar population. The disk component shows hints of spiral structure, though details are limited. A significant portion of the galaxy's light is concentrated along the plane of the disk. The overall color appears yellowish-white, suggestive of a mix of stellar populations, with a predominance of older, evolved stars. There is some evidence of patchy regions within the disk that are slightly bluer in color, potentially indicative of ongoing star formation. There may be some dust lanes present that are obscuring the light emitted from stars. Overall, there are no strong signs of disruption or major tidal interactions in this galaxy.
