The galaxy presents a complex morphology, suggestive of an interacting or merging system. There appears to be at least one dominant core exhibiting a relatively smooth, centralized concentration of light. This core is surrounded by a more diffuse halo of fainter light. There is evidence of tidal features, specifically a plume-like extension, emanating from one side of the galaxy. This may indicate a past or ongoing gravitational interaction. The overall color is slightly blue-shifted on one side compared to the core of the galaxy, possibly hinting at ongoing star formation within the tidal arm or disruption in one portion of the galaxy. Further analysis would be required to determine the nature of the interaction and the ages of the stellar populations within the galaxy.
