This galaxy presents as a moderately inclined spiral, exhibiting a clearly defined disk structure. Spiral arms are apparent, though somewhat flocculent in appearance, indicating potentially ongoing star formation regions along their length. The spiral arms appear to exhibit an intermediate winding, not tightly wound but also not widely dispersed. There might be up to 4 spiral arms. A small, but well defined bulge is visible. The galaxy's central region presents a prominent bar feature, extending across a significant portion of the galaxy's diameter. The galaxy shows evidence of possible interaction or merging activity, presenting a distorted structure possibly due to the influence of another galaxy. The disk demonstrates an irregular morphology, which is consistent with tidal interactions disrupting its normal spiral form. Some color variation is visible, which may indicate differences in stellar populations across the galactic disk.
