The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a notable elliptical morphology, appearing more elongated than perfectly circular. The central bulge is prominent and displays a yellowish-orange hue, suggesting a population of older stars. A fainter, disk-like structure appears to extend outward from the core, primarily along the major axis. There is some subtle bluer light to the side, possibly signifying younger stars or a faint spiral arm segment. The overall structure hints at a relatively undisturbed system, though the faint asymmetric light may indicate a possible past or minor interaction.
