The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core region exhibits a bright, yellow-white hue, suggesting an older stellar population dominating the light emission. There are suggestions of faint, disk-like structures or tidal tails surrounding the central bulge, possibly indicating recent or ongoing interactions. The outer regions transition into a fainter, diffuse halo. Colors are relatively uniform across the galaxy, though there may be regions of blue light indicating younger star formation. There is no strong evidence of spiral arm structure or a prominent dust lane. The overall appearance suggests a fairly evolved system. 
