The galaxy presents as an elliptical morphology, exhibiting a generally smooth light distribution. The central region displays a higher surface brightness, appearing more concentrated. The galaxy's shape is elongated, with a cigar-like appearance; it does not appear perfectly spherical. There's a suggestion of a faint disk or a more extended, diffuse component surrounding the central bulge. The overall color gradient suggests older stellar populations are more dominant, with a reddish-yellow hue in the core that fades into a slightly bluer halo. There are no obvious signs of ongoing major mergers or significant tidal disturbances, and the overall structure appears relatively undisturbed.
