The galaxy appears to be undergoing a significant interaction, showing evidence of a possible merger. The central region presents a bright, concentrated core, suggesting a high density of stars or an active galactic nucleus, and it's shape is complex. A plume or tidal tail is present, extending from the main body, indicative of gravitational disruption. There is a slight color variation within the galaxy, with hints of bluer regions possibly indicating areas of ongoing star formation, though the overall color leans toward the redder end of the spectrum. The overall morphology is complex and irregular, with a disturbed shape.
