The galaxy presents a generally smooth, elliptical morphology. Its color profile suggests a dominant population of older stars, indicated by a yellowish-red hue. There is a lack of distinct spiral arm structures or prominent dust lanes, further supporting its classification as an elliptical galaxy. The overall light distribution is centrally concentrated with a gradual decrease in brightness outward from the core, appearing mostly undisturbed with no obvious signs of ongoing major mergers or tidal interactions. This implies a relatively quiescent evolutionary state. The roundness of the galaxy suggests an E4 or E5 classification on the Hubble sequence, as it shows a moderate departure from perfect sphericity.
