The galaxy presents as an elliptical or lenticular morphology, exhibiting a smooth light distribution with no apparent spiral arms or distinct features. It displays a concentrated central bulge, fading outwards into a more diffuse halo. The galaxy appears to be generally round in shape, with a slight suggestion of being somewhat flattened. There is no obvious evidence of ongoing major mergers or significant tidal disturbances. The colors suggest moderate star formation, with the overall light output indicating that it is a relatively massive galaxy.