The galaxy presents as a relatively smooth object with a centrally concentrated luminosity profile. The overall shape appears to be roughly elliptical, tending toward a more rounded appearance, though some asymmetry is present. The central region exhibits a yellowish-white hue, possibly indicating an older stellar population. The outer regions are fainter and show a bluer tint, suggestive of the presence of younger stars or ongoing star formation, although the blue component is not strongly dominant. No prominent spiral arms or bars are evident, and there's no clear indication of any major ongoing merger activity or significant morphological disturbance. The galaxy is a moderate distance, and its light is redshifted. 
