The galaxy presents as a generally smooth, elliptical morphology. It is dominated by a centrally concentrated spheroid with a relatively high degree of circularity in its overall shape. The light distribution appears uniform across the galaxy, with no discernible spiral arms, bars, or prominent dust lanes. The core region appears to be bright and compact, indicative of a high stellar density.

The color profile suggests a population of older stars, consistent with a relatively low star formation rate. There is a subtle color gradient across the galaxy, possibly indicating differences in stellar populations between the core and outer regions, though this is minimal. There are no prominent signs of recent or ongoing mergers or tidal disturbances, maintaining a regular shape with no obvious distortions.
