The galaxy presents as a relatively compact object with an apparent elongation, suggesting a disk-like structure viewed at an angle. The central region exhibits a brighter, smoother appearance, possibly indicating a bulge component. A faint, diffuse tail-like feature extends from the central region, potentially a tidal feature resulting from past interaction, or some other kind of disturbance. Color gradients are present across the galaxy, with the central region appearing bluer than the outer regions. The bluer color may indicate the presence of younger, hotter stars in the central areas. Overall, the object appears to be a somewhat disturbed galaxy, showing signs of a possible minor interaction or merger event, although the overall structure remains somewhat intact.
