The galaxy appears to be undergoing a merger or significant interaction with a smaller companion galaxy. The primary galaxy presents a relatively smooth, elliptical-like morphology, with a concentrated central bulge that emits strongly. A secondary, smaller object is positioned close to the primary galaxy, suggesting a physical association. The overall color is yellowish-orange, indicative of an older stellar population. The galaxy exhibits a moderate level of star formation. There is some degree of disturbance in the overall morphology.