The galaxy appears to be an elliptical galaxy, exhibiting a smooth, spheroidal morphology. It presents a concentrated central bulge that dominates the overall structure. The galaxy's color profile suggests a population of older stars, indicated by the yellowish hue, indicative of evolved stellar populations. There appears to be no significant dust lane or spiral arm structure, consistent with a relatively quiescent system with limited ongoing star formation. The galaxy exhibits a high degree of circularity. There are no obvious signs of major mergers or tidal disturbances.
