The galaxy appears to be a relatively smooth, elliptical galaxy. Its overall shape is slightly elongated, but it is mostly round. There is a concentration of light towards the center, which suggests the presence of a galactic bulge. The galaxy exhibits a colour gradient, transitioning from a reddish hue towards the core to a bluer tint in the outer regions. This may indicate a difference in stellar populations, with older, redder stars concentrated centrally and younger, bluer stars populating the outer areas. There is no evidence of strong spiral arm structure or significant dust lanes, but there is a hint of a very faint disk. There is no obvious sign of major mergers or tidal disturbances.
