The galaxy presents as an elongated, cigar-shaped structure, likely a flattened elliptical or an edge-on spiral. The central region exhibits a higher surface brightness, appearing more concentrated. The color distribution suggests an aging stellar population, with a reddish-yellow hue dominating the core and inner regions. There is faint evidence of bluer light in the outer edges of the galaxy, suggesting on-going star formation, albeit at a lower rate compared to the central bulge. The galaxy appears relatively undisturbed, with no major signs of tidal interactions or merging events. 
