The galaxy exhibits a complex morphology, suggestive of an ongoing or recent merger event. The system presents with a dominant, relatively smooth and centrally condensed component. A smaller, less distinct component is observed in close proximity, showing some evidence of tidal interactions or disturbance to its morphology. The primary body appears somewhat elliptical, however, the secondary component and possible tidal features disrupt the overall smooth appearance. The system has a yellow-red hue. Given the redness, and relatively smooth appearance of the primary galaxy, it is likely an older system that has largely ceased star formation. The presence of a secondary component increases the probability of recent or ongoing interactions between the two galaxies.
