The galaxy presents as a moderately bright, elliptical-like structure. It exhibits a centrally concentrated luminosity profile, with the brightest region residing in a well-defined core. The isophotes appear to be relatively smooth and regular, indicating a lack of significant ongoing mergers or major tidal disturbances. The overall color is moderately red, suggesting an older stellar population and suppressed star formation. There may be a faint, diffuse halo extending beyond the main body of the galaxy, though the contrast is low. The galaxy is well-defined from the background.
