The galaxy appears to be an elliptical galaxy, characterized by a smooth, diffuse light distribution without prominent spiral arms or a well-defined disk structure. It exhibits a slightly elongated shape, neither perfectly spherical nor highly flattened. A bright, concentrated central bulge is evident, indicative of a high stellar density in the core. The galaxy displays a color gradient, with the central bulge appearing yellower, suggesting an older stellar population dominated by redder stars, while the outer regions exhibit a slightly bluer hue, possibly indicating the presence of younger, bluer stars or ongoing star formation. There is no strong indication of any major mergers or tidal disturbances in its morphology. The general structure appears relatively undisturbed, representing a galaxy that has likely undergone significant evolution and stabilization over time.
