The galaxy presents as a generally smooth, elliptical structure. It exhibits a central bulge that is noticeably brighter and has a more yellow-orange hue, suggesting an older stellar population dominating the core. The outer regions display a slightly bluer tint, which may indicate the presence of younger stars or ongoing, albeit low, levels of star formation. The overall shape is elongated, leaning toward a cigar-like morphology. There are no obvious signs of major mergers or significant tidal disturbances, although subtle asymmetries in the outer regions may indicate minor interactions. The galaxy displays a relatively compact size. 
