The galaxy presents a primarily smooth morphology with an elliptical shape. The central bulge exhibits a concentrated, bright orange-red hue, suggestive of an older stellar population. This core region transitions to a fainter, blue-tinged disk extending outward. A subtle asymmetry is apparent, potentially indicative of minor gravitational interactions or internal disturbances. The galaxy appears to be actively undergoing some level of star formation, as implied by the bluer color in the disk. The overall form indicates a system somewhere between a pure elliptical and a spiral galaxy. There is a possibility of a merger event in its past, or currently in progress.
