The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high concentration of luminosity, appearing bright and yellowish-white, suggesting an older stellar population. There is a subtle color gradient moving outwards from the core, shifting to a slightly bluer hue in the outer regions. No distinct spiral arm structure or significant dust lanes are visible. The overall shape is generally round. There are no obvious signs of major tidal disturbances or ongoing mergers, but the possibility of minor interactions cannot be ruled out based on the image alone. The estimated size is a few kiloparsecs in radius. The galaxy appears to be undergoing a low rate of star formation.
