The galaxy presents as a single, dominant object with an elliptical morphology. Its overall structure is characterized by a smooth light distribution, appearing mostly uniform. A slight color gradient is visible, shifting from a somewhat bluer hue in the outer regions to a yellower tone towards the central core. This color difference suggests possible variations in stellar populations, with potentially younger, bluer stars residing in the outer parts and older, redder stars concentrated in the center.

The galaxy does not appear to have any signs of major disturbances or ongoing mergers. There are no tidal tails, bridges, or other obvious signatures of gravitational interactions. The galaxy's symmetry seems undisturbed.
