The galaxy presents as a somewhat lenticular or early-type spiral morphology, though the arms are not clearly defined. The central bulge is prominent and exhibits a yellowish-white hue, suggesting an older stellar population. Extending outward from the bulge, there's a hint of a flattened disk structure. Faint bluish regions are observed within the disk, which could indicate areas of ongoing star formation. The overall shape appears elongated, possibly cigar-shaped. There seems to be some evidence of minor gravitational disturbance on the bottom of the galaxy.
