The galaxy appears to be a relatively smooth, elliptical or lenticular type. Its light distribution presents a centrally concentrated bulge region with a generally diffuse, extended halo. There is no obvious presence of spiral arms or significant dust lanes. The galaxy exhibits a nearly circular morphology, with a slight deviation hinting at a possible minor interaction or internal asymmetry. The color distribution is characterized by a redder central region, indicative of an older stellar population, transitioning to slightly bluer hues in the outer regions, suggesting the presence of some younger stars, though overall star formation seems relatively low. There is no clear evidence of a major ongoing merger, although some minor disturbances cannot be ruled out based on the overall morphology.
