The galaxy presents as a moderately luminous, likely elliptical or lenticular galaxy. Its morphology appears predominantly smooth, with no discernible spiral arms or bar structure. The overall shape is somewhat elongated, leaning towards an intermediate ellipticity. The light distribution indicates a central bulge that is bright and relatively concentrated, surrounded by a more diffuse halo. There is no strong evidence of ongoing major mergers, tidal tails, or significant disturbances in the galaxy's structure. Some minor asymmetry or possible disturbance is suggested in one quadrant. Its color is primarily consistent with an older stellar population, suggesting relatively low current star formation activity.