The galaxy exhibits a morphology consistent with an ongoing or recent merger event. The main body appears somewhat amorphous, with a bright central condensation and what seem to be two distinct luminous clumps interconnected by a fainter bridge of light. It displays a generally smooth appearance overall, but the asymmetry and the presence of multiple luminous regions suggest tidal interactions are occurring or have recently concluded. The central condensation is dominant and relatively rounded. There are some indications of minor disturbances in the galaxy's overall structure beyond the two distinct regions. A faint extension or tidal tail appears to emanate from the side of the galaxy. The color of the light suggests it may be an old galaxy without much ongoing star formation.
