The galaxy presents as an elliptical structure with a smooth, centrally concentrated light distribution. The core region exhibits a bright, relatively compact profile, suggestive of an older stellar population. Proceeding outwards from the core, the light gradually diminishes into a faint, diffuse halo. There are no visible spiral arms, bars, or distinct dust lanes. A slight elongation is observed. There is no indication of any major ongoing merging activity or tidal disturbances, but there could be some minor asymmetry. The color indices suggest that the galaxy is composed predominantly of older, redder stars, consistent with a low rate of star formation.
