The galaxy presents as a relatively smooth, elliptical-like structure, with a concentrated central bulge that emits a yellowish hue. Moving outwards from the center, the light becomes increasingly diffuse and the galaxy gradually fades into the background sky. The overall shape is elongated, appearing cigar-shaped, suggesting an oblate spheroidal morphology. There are no prominent spiral arm features or significant dust lane obscuration evident in this image. The galaxy appears relatively undisturbed, with no obvious signs of recent or ongoing major mergers. There might be a minor disturbance in the symmetry of the outskirts, although it's hard to tell from the image. Star formation may be happening but at a lower rate than what we see with spiral galaxies. 
