The galaxy presents as a concentrated, centrally brightened object with a generally smooth appearance. The central region exhibits a high degree of symmetry, appearing almost circular. A subtle radial gradient is apparent, with luminosity decreasing from the center outwards. Some indication of subtle disturbances or faint features are visible in the outer regions of the halo, with small changes in the overall smooth light distribution, which is indicative of possible tidal interactions. The galaxy's color appears overall yellowish to reddish. This suggests a population of older stars, indicating a lack of significant recent star formation activity.
