The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge region displaying a reddish hue, potentially indicating an older stellar population. The galaxy fades into a faint green-blue halo, which is likely from recent bursts of star formation. The overall shape is somewhat elongated, but it lacks any obvious signs of spiral arms or major disturbances. There are no prominent tidal tails or other features that would suggest a recent major merger event. A minor disturbance cannot be ruled out due to the slight distortion in morphology. The absence of distinct features suggests a system dominated by older stars and relatively low ongoing star formation activity.
