The galaxy presents a largely smooth morphology. The light is centrally concentrated with a bright nucleus, with a diffuse halo extending outwards. There appears to be minimal, if any, spiral arm structure. The object appears to be an elliptical or lenticular galaxy, exhibiting a relatively round shape, though somewhat elongated. There is little evidence of any major ongoing merger activity. However, there is an asymmetry in the brightness distribution, suggesting a possible minor interaction, or it could be due to internal dust extinction. Color gradients are visible, with the central region appearing more yellow, shifting to bluer hues in the outskirts.
