The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is somewhere between round and elliptical. There is little evidence of spiral arms or a prominent disk structure in this image. The color profile suggests a population of older stars, with a yellowish-red hue dominating the light emitted. The galaxy is reasonably large and appears to have a high stellar mass. There may be evidence of minor tidal disturbances, but no substantial signs of an ongoing merger. Star formation is present, though it is occurring at a relatively modest rate.