The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits a slight ellipticity, deviating marginally from a perfectly circular shape. The color gradient suggests a population of older stars concentrated towards the center of the galaxy, exhibiting a yellowish hue. The outer regions of the galaxy display a somewhat bluer tint, possibly indicating the presence of a younger stellar population. There is no prominent disk structure, spiral arms, or significant dust lane visible in the image. No apparent signs of major interaction or merging activity are observed; the galaxy seems relatively undisturbed. The galaxy is moderately extended, spanning a small but appreciable angular size in the image. There may be the presence of small amounts of ionized gas.
