The galaxy presents as a relatively smooth, elongated object, likely an elliptical galaxy, as the morphology is predominantly smooth. There is a distinct central bulge with a high concentration of light that appears yellow-orange in color, suggestive of an older stellar population. The galaxy displays a slight cigar-shaped morphology.

Based on the color gradients, the outer regions appear bluer compared to the central bulge, which may indicate the presence of some younger stars, although they do not dominate the overall color profile. There are no clear signs of spiral arms, bars, or significant dust lanes. No significant mergers or disturbances are observed, although minor interactions cannot be ruled out. 
