The galaxy presents a largely smooth and rounded morphology. It appears to be elliptical or lenticular in nature, exhibiting a concentrated central bulge that transitions into a diffuse outer halo. There is a slight deviation from perfect circularity; it could be classified somewhere between round and slightly elongated. Overall, the galaxy appears relatively undisturbed, with no major signs of ongoing or recent merger activity. The color profile suggests a predominantly older stellar population. The central region displays a yellowish hue which indicates the presence of evolved stars. The outer regions have a very slight redder tint. Star formation activity is likely low.
