The galaxy presents a generally elliptical morphology with a smooth appearance. The galaxy's central region exhibits a yellow-orange hue, suggestive of an older stellar population. Moving outward from the center, a slightly bluer coloration emerges, hinting at the presence of some younger stars and potential ongoing star formation. The overall light distribution is concentrated towards the center, with a gradual decrease in brightness at larger radii, indicating a well-defined structure without significant tidal disturbances or asymmetries. The shape deviates slightly from perfectly circular, appearing somewhat elongated along one axis. Based on color distribution, the galaxy could potentially be classified as a lenticular or early-type spiral galaxy, viewed at an oblique angle.
