The galaxy presents as a centrally concentrated elliptical system. Its overall structure appears smooth and featureless, with no readily apparent spiral arms or distinct dust lanes. The central region exhibits a bright, compact core that gradually diffuses outwards. The light distribution suggests a relatively old stellar population, indicated by the reddish-yellow hue dominant throughout the galaxy's body. There is a slight elongation in the galaxy's shape, indicating a deviation from perfect circularity. No signs of ongoing major mergers or tidal disturbances are discernible; however, minor asymmetries in the outer isophotes might suggest past interactions. Overall, the galaxy appears as a massive, quiescent system undergoing minimal star formation currently.
