The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated light distribution. There is a lack of prominent spiral arms or a well-defined disk structure. The galaxy exhibits a moderate ellipticity, appearing more lenticular than perfectly spherical. A subtle color gradient can be discerned, with the central regions exhibiting a slightly bluer hue that fades into more red in the outer halo, suggesting potential ongoing, low-level star formation. No major signs of recent or ongoing mergers are visible. There are no significant tidal tails, bridges, or other indicators of strong gravitational interaction. The galaxy is moderately luminous. Overall, the galaxy presents as a relatively quiescent and evolved system.
