The galaxy appears to be a relatively smooth, elliptical or lenticular type. It presents a centrally concentrated light profile, with a gradual decrease in luminosity outwards. There is little to no evidence of spiral arm structure or prominent dust lanes. The galaxy has a generally round appearance, with a slight elongation that could suggest it is more lenticular than purely elliptical. The color appears to be relatively uniform across the galaxy, with a subtle bluer hue towards the center and a slight shift towards redder hues in the outer regions. There is no obvious evidence of major ongoing mergers or strong tidal disturbances. Minor irregularities or subtle features might be present upon closer inspection with higher resolution imaging.
