The galaxy presents a smooth, elongated morphology. It exhibits a cigar-like shape, displaying a significant axis ratio. The color profile suggests an older stellar population, particularly in the central regions. The central bulge is prominent, appearing relatively bright and concentrated compared to the fainter, more diffuse outer regions. There's no strong evidence of spiral arm structure or significant dust lanes. The overall appearance indicates a system with minimal ongoing star formation and a substantial stellar mass. There are no obvious signs of major mergers or significant tidal disturbances. Faint wisps or extensions may be present in the outskirts, but these are subtle.
