The galaxy presents as a single, largely featureless object. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards, displaying a roughly circular shape. There may be a disk component; however, the overall appearance is dominated by a spheroid. Coloration appears relatively uniform across the galaxy, with a general reddish/yellowish hue, suggesting an older stellar population. There is no readily discernible spiral structure or significant dust lane. The galaxy appears relatively isolated and shows no strong evidence of recent or ongoing mergers.
