The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated, bright central bulge that gradually fades into a more diffuse halo. The overall color is yellowish-white, suggesting an older stellar population with fewer young, massive stars. There is no evidence of spiral arms or a significant disk component. The galaxy shows a high degree of central concentration and rotational symmetry. There are no apparent signs of recent mergers or tidal disturbances, and it appears to be an isolated system. Its morphological classification would likely place it along the early-type sequence. Star formation appears to be relatively low, consistent with the color and smooth morphology.
