The galaxy appears to be a relatively smooth, elliptical-type system. It presents with a concentrated central bulge exhibiting a yellow-orange hue, suggestive of an older stellar population. The light distribution is centrally peaked, fading gradually towards the outer regions. There is little evidence of spiral arms or distinct disk structure. The galaxy has a round shape, with only a small amount of ellipticity. No signs of ongoing major merger activity or significant tidal disturbances are apparent, though a slight asymmetry hints at possible minor interactions. The galaxy exhibits a red color, indicating that it is not actively forming many stars.
