The galaxy presents as an apparent merging system, characterized by two distinct components. The primary component exhibits a generally smooth morphology, displaying a nearly elliptical shape. This core appears significantly brighter and more concentrated, with a luminosity that suggests a substantial stellar population. Its color profile indicates a mixture of stellar ages, possibly with a bias towards slightly bluer, younger stars.

The secondary component displays a more diffuse and less well-defined structure. It shows a lower surface brightness compared to the primary galaxy. Its irregular shape hints at gravitational interaction and tidal disruption. There is potential for observable dust lanes and disturbances.

There is visual evidence of an interaction between the components, potentially involving material being exchanged or tidally stretched between the two. This suggests that the system is in a dynamic and evolving state, possibly undergoing a major merger.
