The galaxy presents a complex morphology, appearing as a spiral type with a notable central bulge. The bulge region exhibits a yellowish hue, suggesting an older stellar population. Faint spiral arms are discernible, displaying a slightly bluer color indicative of ongoing star formation regions. The arms are not tightly wound. A possible tidal feature or dwarf galaxy is observed on the left side of the disk. It displays a bluish tint, consistent with star formation. No significant bar structure is clearly visible in the central region. The galaxy overall shows some signs of disturbance, which could point towards a minor merger event in the past. The galaxy disk is not edge-on, but rather at a slight inclination angle.
