The galaxy presents as an elongated structure, exhibiting a cigar-like morphology. The central region is dominated by a bright, yellowish hue suggesting an older stellar population or significant dust obscuration. Moving outward from the center, the color transitions to a bluish-white, potentially indicating younger, hotter stars in the outer regions. The galaxy appears relatively smooth, with only subtle hints of spiral arm structure. The overall shape is suggestive of a late-type spiral galaxy viewed at a high inclination, potentially a lenticular galaxy. There are no obvious signs of a major ongoing merger, though minor disturbances or faint tidal features may be present but are difficult to resolve in this image. The galaxy is moderately luminous and appears relatively massive. It exhibits ongoing star formation.
