The galaxy appears to be a relatively smooth, round object. It exhibits a concentrated central bulge that dominates its overall luminosity. The color profile suggests an older stellar population, with a redder hue observed throughout the galaxy. There is little to no evidence of spiral arms or significant dust lanes. The galaxy appears undisturbed, with no obvious signs of a recent major merger or tidal interactions. The galaxy's size is moderately compact, and its overall structure implies it could be classified as an elliptical galaxy.
