The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and rounded morphology. The central region is very bright, suggesting a high concentration of stars and possibly a supermassive black hole at the galactic nucleus. The light profile fades gradually outward from the center, with no discernible spiral arms or distinct disk features. There is a slight elongation, deviating from a perfect circle, but it's mostly round in appearance. There's no clear evidence of ongoing major mergers or significant tidal disturbances, although some minor irregularities in the outer regions hint at possible past interactions. Based on the color, the galaxy is likely composed of an older stellar population, with relatively little ongoing star formation.
