The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be elliptical in shape, with a slight elongation rather than a perfect circle. The central region exhibits a brighter, somewhat diffuse glow, suggesting a concentrated stellar population or possible active galactic nucleus. Surrounding the core, the galaxy fades gradually outward, indicating a less dense distribution of stars in the outer regions. The overall color profile suggests an older stellar population, potentially with ongoing but subdued star formation, and a substantial mass. There are no distinct spiral arms or bar structures visible, nor any major signs of tidal disturbances or ongoing mergers.
