The galaxy presents an elongated, cigar-shaped morphology. Its central region exhibits a concentrated, yellowish-orange hue, suggestive of an older stellar population, and potentially, ongoing low-level star formation. The outer regions appear fainter with a bluish tint, potentially indicating the presence of younger, hotter stars in the galactic disk. There is no obvious spiral structure discernible at this resolution. The galaxy appears relatively smooth in overall texture, with no apparent major disturbances, or merging events.
