The galaxy presents a spiral morphology, characterized by a relatively small bulge. The spiral arms are tightly wound and well-defined, extending from the central region. Two dominant spiral arms are easily discernable. The disk component shows a range of colors, with bluer regions indicating areas of ongoing star formation. Dust lanes are visible within the spiral arms, contributing to the overall structure. No evidence of major mergers or significant disturbances is observed. The galaxy is not oriented edge-on, allowing for a good view of the spiral structure. A weak bar feature may be present in the central region.
