The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that transitions smoothly outwards. There is little evidence of spiral arm structure or significant dust lanes. The color gradient suggests a population of older stars dominating the galactic light, as indicated by the yellowish hue in the center. The outer regions are fainter and slightly bluer, possibly indicating a small amount of on-going star formation, though the overall signature points to a quiescent galaxy. There are no obvious signs of tidal disturbances or major merger events. The overall morphology suggests it is a mature, relaxed system.
