The galaxy presents as a centrally concentrated, relatively smooth object. Its overall color appears yellowish-white, suggestive of a stellar population dominated by older, less massive stars. The morphology is largely elliptical or lenticular, with a high degree of central concentration and minimal visible substructure. There is very little, if any, evidence of spiral arms or prominent dust lanes. The galaxy exhibits a moderate degree of roundness in its overall shape, and there is no significant tidal distortion or obvious signs of ongoing mergers or major interactions with other galaxies. The light is relatively uniform across the main body of the galaxy, with a slight decrease in intensity towards the outer regions.
