The galaxy presents as a fairly smooth, elliptical structure with a concentrated central bulge. It exhibits a yellowish-orange hue, suggesting a population of older stars. There is little to no evidence of prominent spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, with no obvious signs of ongoing mergers or major interactions. A slight elongation is observable, deviating from a perfectly circular morphology. There is faint suggestion of a disk-like structure, but this feature is poorly defined. No bright knots indicative of star formation regions are readily apparent. Overall, the galaxy appears to be a mature system with limited recent star formation.
