The galaxy presents as an elliptical morphology, with a smooth and somewhat elongated profile. Its central region exhibits a concentration of light, appearing significantly brighter and more yellow-orange than the outer regions. The color gradient suggests a dominant population of older stars within the core. The periphery of the galaxy fades gradually into the background, lacking any distinct or sharp edges, further reinforcing the impression of a well-established elliptical structure. There are no visually apparent spiral arms or dust lanes. No obvious signs of recent or ongoing major mergers or tidal disturbances are detected.
