The galaxy presents as a relatively face-on spiral with discernible arm structure. The arms appear somewhat patchy and loosely wound, indicative of ongoing star formation. A central bulge is not prominently visible, suggesting a smaller or less dense stellar population concentrated at the core. The overall color of the galaxy leans towards a bluish hue, particularly within the spiral arms, hinting at a significant population of young, hot stars. There is evidence of tidal disturbances, with a notable amount of asymmetry, it is potentially interacting or undergoing a merger event, with diffuse and disturbed morphology. There is a bar-like structure across the galactic center.
