The galaxy presents an elongated, cigar-shaped morphology, indicative of a disk galaxy viewed at a high inclination. The central bulge appears relatively bright and smooth, with a concentrated luminosity profile, possibly suggesting an older stellar population. The disk is characterized by a faint, diffuse blue hue, suggestive of ongoing, but not highly vigorous, star formation. There is no evidence of strong spiral arm structure or major disturbances from mergers or tidal interactions, though some subtle asymmetry exists within the disk. The overall structure appears largely undisturbed and relatively quiescent.
