This galaxy exhibits a morphology suggestive of an ongoing or recent interaction. Two distinct luminous regions are visible, indicating potentially two galactic nuclei in the system. The overall form is somewhat amorphous, lacking a clearly defined spiral or elliptical structure. A faint, diffuse halo of light surrounds the primary luminous regions, potentially indicating tidal debris resulting from gravitational interactions. The color profile appears relatively uniform across the galaxy, with a slight redder hue overall, which could suggest a relatively older stellar population and low levels of active star formation. Faint tidal tails might be present but are not distinct, possibly further evidence of a past merger event. The size of the system is considerable, occupying a notable portion of the field of view.
