The galaxy presents as a largely smooth, elliptical structure. It exhibits a moderate elongation, appearing somewhat cigar-shaped. The galaxy's color gradient transitions from a warmer, yellowish hue at its core to a subtly cooler, bluer shade towards its outer regions. There is no readily apparent spiral arm structure or significant dust lane obscuration. The galaxy seems relatively undisturbed, with no major signs of an ongoing merger event, although a minor tidal disturbance cannot be completely ruled out. The overall morphology suggests a system dominated by an older stellar population with a low current star formation rate. The effective radius, judging by the apparent size in the image, is moderate, suggesting it is a reasonably sized galaxy.
