The galaxy appears to be a relatively smooth, centrally concentrated object. The light profile suggests a dominant spheroidal component. There is little evidence of strong spiral arm structure or prominent dust lanes, leading to a morphological classification leaning towards elliptical or lenticular. The galaxy exhibits a color gradient, with a slightly yellower or redder hue towards the center and a bluer tint in the outer regions. It does not seem to be undergoing any major mergers or tidal interactions based on the image.
