The galaxy appears to be a spiral galaxy, exhibiting a clear disk structure with prominent spiral arms. The arms are tightly wound and exhibit a noticeable blue hue, indicative of ongoing star formation. A central bulge is present, though it seems to be of moderate size, with the disk dominating the overall structure. There is no strong evidence of a bar structure. The galaxy appears relatively undisturbed, with no major signs of a merger or tidal interactions. The galaxy is observed at a slight inclination, allowing a clear view of the spiral structure.
