The galaxy presents as a relatively smooth, elliptical-like structure, displaying a concentrated central bulge that appears to be yellowish-white. The outer regions of the galaxy fade gradually into the background sky, exhibiting a faint bluish-white hue. There are no prominent spiral arms or distinct dust lanes visible in this image, suggesting a more evolved stellar population. The overall morphology indicates a system with a dominant spheroidal component. The galaxy's shape is somewhat elongated but still generally rounded. There is no visible evidence of a major ongoing merger or significant tidal disturbance, though a subtle asymmetry cannot be ruled out. Based on the color and morphology, this galaxy could be a massive system, likely with low ongoing star formation.
