The galaxy presents as a moderately luminous object with an elliptical morphology. It exhibits a relatively smooth light distribution, lacking prominent spiral arms or a distinct disk structure. The galaxy appears approximately circular in shape, with a slight tendency towards elongation. The core region shows some concentration of light, although it is not excessively bright or indicative of an active galactic nucleus. There is no noticeable presence of tidal tails, distorted features, or signs of recent major merger activity. The overall color is consistent with an older stellar population.
