The galaxy presents as a single, largely featureless, centrally concentrated object. Its overall color appears to be a yellowish-orange hue, suggesting a population of older stars and a relative lack of ongoing star formation. The morphology indicates a spheroid shape with a high degree of symmetry. There are no discernible spiral arms, bars, or tidal features indicative of recent mergers or significant gravitational disturbances. The light is centrally concentrated, with a smooth and gradual decline in surface brightness from the core outwards. The lack of obvious blue regions suggests minimal ongoing star formation, and the redder color indicates a stellar population dominated by older, cooler stars.
