The galaxy presents as an elliptical morphology, appearing largely smooth and centralized. Its light profile suggests a dominant, well-defined core, with a gradual decrease in luminosity towards the outer regions. There are some suggestions of bluer colors at the edge of the light suggesting some limited star formation present. The overall color appears to be relatively consistent with an older stellar population; the central core presents a yellowish hue, indicative of evolved stars. No prominent spiral arm structures or dust lanes are discernible, furthering the categorization as elliptical. The galaxy is of intermediate apparent size. There is no obvious evidence of any major ongoing mergers or significant tidal disturbances affecting its overall structure.