The galaxy presents as a spiral type with a noticeable disk structure. The arms are well-defined but possess a flocculent morphology. The winding of the arms appears loose. A central bulge is prominent and accounts for a significant portion of the galaxy's luminosity. The color gradient indicates an older stellar population concentrated in the bulge, transitioning to bluer hues along the spiral arms, suggesting ongoing star formation. The galaxy exhibits a relatively high inclination angle with respect to our line of sight. There is no apparent bar structure. Based on the disturbances in the spiral shape of the galaxy, it might be interacting with smaller objects nearby.
