The galaxy presents a generally smooth, elliptical morphology. The central region displays a concentrated, bright, yellowish-orange color, indicating an older stellar population likely dominated by evolved stars. Moving outwards from the core, the galaxy's color gradually shifts toward a bluer hue, suggesting the presence of a younger stellar population in the outer regions, possibly indicating ongoing or recent star formation. No distinct spiral arms or bar structures are discernible. The galaxy's shape appears somewhat elongated but mostly rounded. There are no visually apparent signs of significant tidal disturbances or ongoing mergers, though the galaxy's asymmetrical overall shape suggests the possibility of a past interaction or minor disturbance.
