The galaxy presents a morphology that is largely smooth and elliptical. The central region exhibits a bright, concentrated luminosity profile, with a color gradient suggesting an older stellar population. The isophotes appear generally regular, indicating a relaxed dynamical state. The galaxy appears relatively isolated, with no obvious signs of major mergers or tidal disturbances in its immediate vicinity, though minor disturbances may be present. The overall color is redder, possibly due to a lack of significant recent star formation. The estimated size indicates a relatively compact galaxy.
