The galaxy presents an elliptical morphology, elongated along its major axis. A bright, concentrated central bulge is prominent, indicating a high stellar density in the core. The color gradient transitions from a yellow-white center to a redder periphery, potentially indicative of older stellar populations in the outer regions. A hint of dust lanes, possibly associated with on-going or past minor mergers, are visible. Overall the galaxy appears relatively undisturbed, showing no strong signs of tidal features or recent major merger events. The estimated size of the galaxy would be approximately 3.5 kpc. The rate of star formation is low. The galaxy's estimated mass is very high.