The galaxy presents a largely smooth, elliptical morphology. It appears as a concentrated central bulge, with a gradual decrease in luminosity towards the outer regions. The core exhibits a strong reddish-orange hue, suggesting an older stellar population. Fainter, diffuse greenish-blue areas can be discerned around the central bulge, potentially indicative of sparse regions with ongoing star formation. The overall shape is generally circular, with no apparent major distortions or tidal features suggestive of recent major mergers. A very faint, extended halo surrounds the main body of the galaxy. The galaxy appears relatively isolated.
