The galaxy presents a generally smooth and elongated morphology, indicative of an elliptical or lenticular type. The central region exhibits a high concentration of light, appearing as a bright, yellowish core, suggesting a population of older stars. Moving outward from the center, the light gradually diminishes, forming a diffuse halo with a bluish tint. The overall structure is relatively undisturbed, though there might be a slight asymmetry or faint tidal features hinting at possible past interactions. There is a suggestion of a disk, but no spiral structure is visible. The color gradient indicates a spatial variation in stellar populations, with bluer stars potentially residing in the outer regions and older, redder stars dominating the core.
