The galaxy presents as a spiral type, observed nearly face-on. Distinct spiral arm structures are visible, displaying a multi-armed morphology, most notably featuring three spiral arms. The arms exhibit a relatively tight winding pattern. A central bulge is apparent, contributing substantially to the overall light profile of the galaxy and exhibiting a moderate size. The image suggests that a bar structure may be present, though it appears weak. No significant tidal features or strong signs of interactions are observed, though subtle disturbances may be present. The galaxy exhibits an apparent star formation activity based on its colors, and would seem to have an approximate diameter of 5 kpc.
