The galaxy presents an overall smooth morphology, suggesting a classification as an elliptical galaxy. Its shape appears mostly round with only slight deviations from a perfect circle. There is little indication of spiral arms or significant disk features. The central bulge is prominent and relatively bright, displaying a yellowish-white hue, possibly indicative of an older stellar population. The outer regions exhibit a bluer color, hinting at the presence of some younger stars or ongoing, albeit subdued, star formation. There is no obvious evidence of a major merger or significant tidal disturbances, though subtle irregularities may indicate minor interactions. The galaxy's relatively compact size suggests it is not a large, extended system. 
