The galaxy appears as a smooth, elliptical-like structure with a concentrated central bulge. There are no discernible spiral arms or a distinct disk. The galaxy exhibits a yellow-orange hue, indicating a stellar population dominated by older stars. The light is relatively uniform across the galaxy, with a slight increase in intensity towards the center, suggesting a higher concentration of stars in the core. There is a small, faint, diffuse region near the galaxy's main body, it is unclear if this is tidal debris, a minor disturbance, or simply noise in the image. There are no other indications of active galactic nuclei or significant ongoing star formation.
