The observed galaxy presents a notable elliptical morphology. It exhibits a relatively smooth and concentrated light profile, transitioning gradually from a bright central nucleus to a fainter extended halo. The central region appears yellowish, potentially indicating an older stellar population. There is no discernible spiral arm structure or significant dust lane obscuration. The overall shape leans towards being 'in between' round and elongated. The galaxy appears relatively undisturbed, showing no significant signs of ongoing major merger activity, although there seems to be a minor disturbance along the disk.
