The galaxy presents as a relatively smooth, centrally concentrated structure. It appears to be an elliptical galaxy exhibiting a spheroidal morphology. The core region shows a bright, concentrated luminosity profile suggestive of a high stellar density. Moving outwards from the core, the light intensity gradually decreases, forming a diffuse halo. There is some visual evidence of a very subtle disk structure. There is no apparent sign of significant dust lanes or prominent spiral arm features. There is no indication of a major ongoing merger, but potentially minor signs of tidal disturbance. The overall color appears to be yellowish-orange, consistent with an older stellar population and a relatively low rate of recent star formation.
