The galaxy presents as a spiral type, exhibiting prominent disk features. There is a definite disk structure with hints of spiral arm morphology. The galaxy appears inclined to our line of sight, providing a near edge-on view. The central bulge appears relatively smooth and elongated. The spiral arms exhibit clumpy structures, suggesting active star formation regions. The galaxy shows signs of potential disturbances, as indicated by the slightly asymmetric arm structure and a faint tidal tail. The color distribution indicates the presence of both older stellar populations, dominating the bulge, and younger, bluer stars within the spiral arms. There may be a relatively modest rate of star formation. Overall, the galaxy appears to be a spiral undergoing some form of interaction or internal disturbance.
