The galaxy presents a generally smooth and elliptical morphology, appearing relatively featureless at this resolution. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. There is a subtle disk-like structure with no visible spiral arms. Its color suggests an older stellar population, possibly dominated by evolved stars. There are no signs of active star formation, with the overall color profile leaning toward redder wavelengths. There is some indication of a minor gravitational disturbance in the galaxy's shape, but the galaxy is generally isolated and exhibits no signs of a major ongoing merger or strong tidal interactions. 
