The galaxy presents a somewhat irregular morphology. There is evidence of disk features, though possibly viewed at a significant angle from edge-on. A disturbance to the galaxy's shape suggests a possible interaction with a smaller companion galaxy, a past merger event, or strong tidal effects. The galaxy exhibits a noticeable blue tint, indicative of active star formation within. The estimated half-light radius suggests a relatively compact structure, though its morphology is not simply that of a smooth elliptical galaxy.
