The galaxy appears as a fairly smooth, elliptical or lenticular object. It exhibits a central bulge that is bright and concentrated, with a gradual decrease in luminosity towards its outer regions. The overall shape is quite round, with minimal deviation from a circular form. There may be very faint suggestions of spiral arms or a disk structure, but these are not clearly defined.

The color profile is relatively uniform, with a slightly bluer hue in the central region that shifts to a redder tone moving outwards. This suggests ongoing or recent star formation occurring within the inner regions of the galaxy. There are no obvious signs of a major merger event or significant tidal disturbances in the image. The galaxy's structure suggests that is is likely a relatively evolved system that is undergoing steady state star formation.
