The galaxy presents a complex morphology, suggestive of a late-type spiral or potentially a merging system. The central region exhibits a bright, somewhat elongated core, possibly indicating the presence of a bar structure, or a recent merger.

Distinct spiral arms are visible, though somewhat flocculent and disrupted. The arms are traced by regions of bluer light, suggesting active star formation. Patches of redder hues are dispersed along the arms, likely corresponding to older stellar populations or dust lanes.

The galaxy shows hints of disturbance in its overall structure. The distribution of light is not entirely smooth or symmetrical, and there is some irregularity in the shape of the arms. This could be indicative of a minor interaction or merger event.

The galaxy is primarily face-on, allowing for clear observation of its disk structure. The relative size of the bulge seems small compared to the overall extent of the disk.
