The galaxy presents as a largely featureless, smooth elliptical structure. The core exhibits a concentrated, bright luminosity, indicative of a high stellar density and potentially the presence of an active galactic nucleus. The light profile appears roughly spheroidal, transitioning smoothly from the bright central region to a more diffuse outer halo. There is little evidence of spiral arms or distinct dust lanes. The color gradient suggests a population of older stars dominating the stellar population, with a relatively redder hue. Minor disturbances or tidal features are not readily apparent. Overall, the galaxy seems to be a mature elliptical system with a relatively high degree of symmetry. 
