The galaxy presents a smooth, elliptical morphology with a cigar-like shape. It exhibits a color gradient, with the central region appearing more reddish-orange, suggesting an older stellar population and/or dust obscuration. The outer regions show a subtle bluish hue, potentially indicating the presence of younger, hotter stars, although this is less prominent, suggesting low levels of on-going star formation. There is no visual evidence of spiral arms, a central bar, or a distinct disk. No signs of major mergers or significant tidal disturbances are observed. The galaxy appears relatively isolated and undisturbed.