The galaxy appears as a relatively smooth, elliptical-like object with a concentrated central bulge. There is a noticeable decrease in surface brightness moving outward from the core. The galaxy exhibits a slight elongation, deviating from a perfectly circular morphology, but is overall fairly round. The color appears predominantly white/blue-ish, suggesting the presence of a population of younger, hotter stars or the presence of an active galactic nucleus. There is no strong evidence of spiral arms or significant dust lanes visible in this image, nor is there evidence of it merging with another galaxy. The overall structure indicates a potentially evolved system.
