The galaxy presents as a luminous, elliptical-like structure. The central region exhibits a high degree of brightness, suggesting a concentrated stellar population and/or active galactic nucleus. Proceeding outwards from the core, the light gradually diminishes. The galaxy's color profile appears generally yellowish-white in the inner regions transitioning to bluer hues in the outer regions. A subtle irregularity is observed in the disk, hinting at a possible ongoing or recent minor interaction. The overall appearance indicates a system that is generally smooth in structure.
