The galaxy presents as a concentrated, centralized mass of light, appearing predominantly smooth in texture. The central region exhibits a bright, yellow-white glow, indicative of a high density of older stars. While not perfectly spherical, its overall shape tends toward roundness, lacking any prominent spiral arm structures. A faint bluish tinge is discernible on the right side of the galaxy, potentially indicating the presence of younger, hotter stars and recent star formation in that localized area. There is no obvious indication of tidal tails or significant morphological disturbances, however, there are features of the galaxy that suggest a very minor interaction. The galaxy's overall light profile suggests an elliptical or lenticular type, with no discernible central bar or spiral pattern.
