The galaxy appears as a relatively smooth, elliptical-like structure. The central region exhibits a concentrated, yellowish hue, suggesting an older stellar population. The outer regions show a gradual decrease in luminosity with a reddish tint, transitioning into the background sky. There is little evidence of spiral arm structures or significant dust lanes, and no indication of active star formation regions. The galaxy's shape is more elongated. It appears to be a relatively isolated system, without any obvious signs of recent or ongoing mergers or tidal interactions.
