The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in surface brightness towards its outer regions. There appears to be very little if any disk structure present. The galaxy's light is dominated by redder wavelengths, with some presence of green likely showing some star formation, suggesting an older stellar population with ongoing moderate levels of star formation in some regions. No clear signs of major disturbances or tidal features indicative of recent major mergers are visible, though very faint hints of minor disturbances or asymmetries are present. The galaxy's shape is more elongated than circular, with a moderate ellipticity. The galaxy seems compact, and there may be an obscured central point source. 
