The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated, bright central bulge that appears yellowish-orange in color, indicating an older stellar population. Surrounding the bulge is a more diffuse, elongated halo that extends further along one axis, suggesting a slightly cigar-shaped morphology. The halo's color is bluer compared to the bulge, hinting at the presence of younger stars or ongoing star formation activity, albeit at a modest rate. There may be a faint dust lane or subtle feature interrupting the smoothness of the galaxy. Overall, the galaxy appears to be an evolved system undergoing low-level star formation.