The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge, slightly elongated in shape. The color is predominantly reddish-yellow, suggesting an older stellar population with fewer young, massive stars. There's a subtle, diffuse halo surrounding the central region, potentially indicative of a broader distribution of stars. There is little to no evidence of spiral arm structure or significant dust lanes. There is no indication of major disturbances or mergers, with the overall structure appearing relatively undisturbed.
