The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is close to circular. There are no distinct spiral arms or a prominent disk visible. The galaxy's light profile appears fairly uniform, suggesting a population of primarily older stars. There are no obvious signs of ongoing major mergers, tidal tails, or significant disturbances in its morphology. The color is somewhat yellow, which also supports an older stellar population. The estimated size is consistent with a galaxy that is larger than the Milky Way. Star formation is low. 
