The galaxy exhibits a complex morphology. It appears to be a spiral galaxy seen at a slight angle. Two spiral arms are visible and winding. A central bulge is present but is not particularly dominant, with the bulge and disk being of comparable size. The color is predominantly bluish, indicative of a population of young, hot stars and ongoing star formation. Evidences suggest this galaxy may be undergoing a merger or interaction with another galaxy, as shown by some distortion. However, the central region displays a relatively smooth profile, without pronounced signs of active galactic nuclei activity. The overall structure presents a dynamic and evolving system, characterized by both established features and signs of ongoing gravitational interaction.
