The galaxy presents as a relatively smooth, elliptical structure. It exhibits a pronounced central bulge, which appears brighter and more concentrated than the surrounding regions. The color gradient suggests an older stellar population within the bulge, trending towards redder hues. The outer regions of the galaxy show a gradual decrease in luminosity, with a more diffuse, less defined edge. There is a slight elongation, giving it a somewhat cigar-shaped appearance. No prominent spiral arms or distinct features are visible, indicating a lack of significant recent star formation. There is no visual evidence of any ongoing major merger events or significant tidal disturbances. The overall morphology is consistent with an early-type galaxy, likely an elliptical galaxy.
