The galaxy presents as a single, relatively smooth light distribution with a concentrated core. There appears to be minimal structure, lacking spiral arms or a prominent bar. The color profile suggests an older stellar population, with a yellow-red hue dominating the core region and a slight decrease in color temperature extending outward. The galaxy is generally circular in appearance. There is no evidence of recent major merger activity or significant tidal disturbances. The overall impression is that of an early-type galaxy.
