The galaxy presents as a largely featureless elliptical morphology. It exhibits a concentrated central bulge, with a gradual decrease in luminosity towards the outer regions. The core appears bright and slightly yellow, with a smooth distribution of light suggesting an older stellar population. The outer regions are less defined and have a bluish hue, possibly indicating the presence of some younger stars or ongoing, albeit low, star formation. There is a slight elongation in its shape, but it does not exhibit any distinct spiral arm structures or significant dust lanes. There are no obvious signs of tidal disturbances or interaction with other galaxies, although there might be faint irregularities suggesting minor past interactions. The galaxy appears relatively isolated in its environment.
