The galaxy presents a somewhat elongated, cigar-shaped morphology. It exhibits a centrally concentrated bulge that appears relatively smooth and featureless. The color profile suggests a redder hue in the central regions, possibly indicating an older stellar population. The outer regions display a bluer tint, hinting at the presence of younger stars, though the overall color is more indicative of an elliptical galaxy. There is no distinct spiral arm structure visible, and the galaxy appears to be isolated, with no signs of major mergers or significant tidal disturbances. A faint, diffuse halo may be present surrounding the galaxy's main body.