The galaxy presents a morphology suggestive of a possible interaction or merger event. One component appears relatively smooth and elliptical in shape, dominating the system's overall light profile. This component displays a centrally concentrated brightness distribution and a generally featureless appearance. Its color is more yellow, indicating an older stellar population and lower ongoing star formation.

A second component is visible, located to the west. This component is more elongated. Its color suggests the presence of a younger stellar population and/or more dust obscuration. The overall system shows signs of minor disturbance, possibly resulting from gravitational interactions that may stimulate localized star formation within the galaxy.

The spatial extent of the galaxy is relatively compact, and the overall system presents a moderate surface brightness. The galaxy appears as a transitioning system, that has components of both being an elliptical and a merging system.