The galaxy presents as a centrally concentrated object with a relatively smooth light distribution, appearing largely elliptical in shape, but with subtle disc-like characteristics. The color gradient suggests a population of older stars dominating the galactic structure, with a possible redder central bulge or core. There is little evidence of significant spiral arm structure or active star formation regions discernible within the galaxy's body. Faint tidal features or minor disturbances might be present, indicating potential past interactions, though the overall morphology seems largely undisturbed. The galaxy exhibits moderate luminosity. Its profile suggests it is likely a fairly massive galaxy with a quiescent star formation rate.