The galaxy presents a flattened, elongated morphology, indicative of an edge-on or highly inclined disk galaxy. Its color profile suggests the presence of both older stellar populations, seen in the central regions, and younger, possibly star-forming regions distributed along the disk. Patches of slightly bluer light are observed throughout the galaxy, suggesting potential locations of ongoing star formation. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. However, there are minor disturbances that suggest some sort of interaction or internal process. The light distribution is generally smooth, indicating a lack of pronounced spiral arms or other major structural features.
