The galaxy presents as a somewhat elongated, disk-like structure viewed at a significant angle, displaying a cigar-shaped morphology. The central bulge exhibits a concentrated, yellowish glow, indicating a population of older stars. The disk appears relatively smooth with hints of subtle blue structures, which might signify pockets of ongoing star formation. Overall, the galaxy seems relatively undisturbed, without major distortions, suggesting a lack of recent major mergers. There are no obvious signs of a strong tidal interaction with other galaxies nearby.
