This galaxy presents a smooth, elliptical morphology with a noticeable cigar-shaped elongation. The galaxy exhibits a central bulge with a yellowish-orange hue, likely indicating an older stellar population. Surrounding the bulge is a less concentrated, bluer disk. A significant amount of the galaxy's light is emitted at wavelengths corresponding to the r-band. The galaxy appears relatively undisturbed, with no prominent signs of ongoing mergers or major tidal disruptions, though minor disturbances cannot be ruled out. Star formation is suspected based on color but the rate of star formation is not high.