The galaxy appears to be a relatively smooth, elliptical system. It exhibits a slightly elongated morphology, being more "in between" round and cigar shaped, rather than perfectly spherical. There is no obvious strong indication of spiral arms or a prominent disk.

Color gradients are subtle. The central region displays a generally redder hue, possibly indicating an older stellar population or greater dust extinction. The outer regions show a faint bluer tinge, hinting at more recent, though not extremely vigorous, star formation occurring.

There are no major signs of significant mergers or tidal disturbances within this image, though some minor irregularities cannot be ruled out, given the resolution.
