The galaxy presents a prominent disk structure with discernible spiral arms. Two primary spiral arms are clearly visible, winding moderately tightly around a central bulge. The bulge appears relatively small compared to the overall disk size. A faint bar-like feature may be present traversing the central region of the galaxy, extending along the major axis of the disk, which is noticeably inclined. Patchy regions of star formation activity, indicated by blue-tinged areas, are apparent within the spiral arms, contributing to the galaxy's overall bluer hue. The galaxy is likely in a relatively quiescent state, as it doesn't display signs of major disturbances or significant mergers with other galaxies, though a possible minor disturbance in one spiral arm is noticed.
