The galaxy presents as a relatively smooth, elongated structure. The central bulge exhibits a yellowish hue, suggestive of an older stellar population. Extending outwards from the central region, the galaxy displays a disk-like morphology, although the arms are not well-defined. There's some subtle bluer component visible in the disk, which could indicate ongoing star formation, although at a low rate. The overall shape is cigar-shaped, and it appears undisturbed with no signs of a major merger. However, the presence of some asymmetrical features might point towards minor gravitational interactions or internal disturbances.
