The galaxy presents as a spiral type, exhibiting a pronounced disk structure. The spiral arms are tightly wound around a central bulge. The bulge appears to be of moderate size in relation to the disk. Within the spiral arms, there are visible regions of active star formation, indicated by their bluish hue. The galaxy does show some evidence of a bar structure crossing through the central bulge. The galaxy appears relatively undisturbed, with no obvious signs of any major merger or significant tidal disruptions. There is a hint of possible minor interaction or disturbance of the outer disk.
