This galaxy appears to be a relatively elongated or cigar-shaped system. Its light profile indicates that it is likely a disk galaxy seen edge-on. The galaxy has a prominent central bulge, but with a smooth structure, which suggests that the galaxy is likely a spiral galaxy with tightly wound spiral arms that are difficult to resolve at this resolution. The presence of bluer light in regions of the galaxy disk suggests active star formation. The disk exhibits some signs of subtle disturbances, indicating potential past or ongoing minor interactions. Overall, it is a relatively normal, though slightly distorted, disk galaxy.
