The galaxy appears to be a relatively smooth, elliptical galaxy with a dominant spheroidal component. It presents a somewhat concentrated central bulge that exhibits a yellowish hue, suggestive of an older stellar population. The outer regions display a gradual decrease in surface brightness, transitioning to a faint, extended halo. There is a subtle hint of bluer colors within the disk component which indicates the presence of some younger stars or ongoing star formation within that region. There does not appear to be any evidence of tidal tails or strong morphological disturbances indicative of any major merger activity. Based on the observed morphology, the galaxy appears to be relatively undisturbed and likely in a state of quiescent evolution.
