The galaxy presents as a smooth, elliptical morphology. It exhibits a concentrated central bulge that appears nearly spherical. The light profile transitions smoothly from the bright core, fading gradually into the outer regions without any distinct spiral arm structures or prominent dust lanes. The color indices suggest a galaxy dominated by an older stellar population, with a relatively low rate of star formation. The overall color is a warm, yellowish hue, indicative of evolved stars. There appears to be no ongoing major merger activity or significant tidal disturbances in the immediate vicinity, though there seems to be a slight asymmetry. The galaxy shows minimal evidence of recent starburst activity and appears to be a fairly quiescent system. 
