The galaxy presents as an object with a somewhat disturbed morphology, possibly undergoing a merger event. The light distribution appears relatively smooth overall, suggesting an older stellar population is dominant, with some indication of disk features. The shape of the galaxy is neither perfectly round nor elongated, leaning towards being in between. There is a noticeable, luminous core with a redder hue, indicative of a region potentially rich in older stars and/or dust obscuration. A less prominent but similarly colored region appears to the left of the main galaxy body. The galaxy is relatively bright, suggesting a significant stellar mass. There are also some blue areas suggesting some recent star formation. Overall, the galaxy appears to be in an intermediate stage of evolution, potentially transitioning from a more active, star-forming state to a more quiescent one, possibly influenced by the ongoing interaction.
