The galaxy presents as a fairly smooth, centralized object. It exhibits a roughly elliptical morphology, with a moderate degree of roundness. No distinct spiral arm structures are visible, suggesting a lack of prominent disk features.

The color profile indicates a concentration of older stellar populations, with a possible slight increase in young stars present. The light distribution is mostly concentrated towards the center. There are no obvious signs of strong tidal disturbances or ongoing major mergers. Indications suggest a relatively low star formation rate.
