The galaxy presents an elliptical morphology, appearing mostly smooth with minimal discernible features. It exhibits a moderate degree of roundness. The light distribution indicates a concentrated central bulge, with the overall color profile trending towards redder hues, suggesting an older stellar population. There is some evidence of minor disturbances in the form of asymmetries within the extended halo, potentially indicative of past or ongoing interactions with other galactic structures. The overall structure appears relatively compact, with no prominent spiral arms or disk-like features visible.
