The galaxy presents as a system with potential interactions or recent merger events. The primary component appears relatively smooth, with a predominantly elliptical morphology. It exhibits a bright, concentrated core, surrounded by a more diffuse halo. There is evidence of tidal features extending outward, suggesting gravitational disturbance.

To the upper right of the central component, there are luminous regions which may be satellite galaxies or tidal debris resulting from interactions with the central galaxy. The color distribution suggests an aging stellar population.

Overall, the galaxy appears to be a complex system undergoing morphological transformation, characterized by relatively low star formation and a significant stellar mass.
