The galaxy presents a distinct, elongated morphology, resembling a cigar shape. It exhibits a bright, centrally concentrated region, likely the galactic bulge. Moving outward from the core, a faint disk structure is observable, though without prominent spiral arm features. A slight blue tinge suggests the presence of some younger stars, but no particularly bright or well-defined star-forming regions are apparent in this image. Overall, the galaxy appears relatively smooth, with no obvious signs of major disturbances such as tidal tails or asymmetrical features.
