The galaxy presents a generally smooth, elliptical morphology with a slight elongation. The central region appears to be more luminous, with a color gradient transitioning to a slightly bluer hue towards the outer regions. There is little evidence of spiral arm structure or significant dust lanes. The galaxy appears relatively undisturbed, showing no strong signs of tidal interactions or major merger events. The overall impression is that of a relatively evolved system, possibly an early-type galaxy with a population of older stars dominating its light output.
