The galaxy appears as a centrally concentrated, smooth object. Its morphology is largely elliptical, exhibiting a high degree of sphericity. There is little to no visible disk structure or spiral arm features. Coloration indicates a prominent bulge with a population of older stars, contributing to the yellowish hue in the central region. The light smoothly fades towards the outer regions of the galaxy, indicating a lack of active star formation in the outer disk or halo, as suggested by its redder color at the periphery. There is no obvious interaction or disturbance present from the image. It seems to be a rather relaxed and undisturbed system.
