The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, with a gradual fading of light intensity moving outwards. The color profile suggests a centrally located population of older stars, indicated by the yellowish hue. A faint, diffuse halo of bluer light surrounds the central bulge, possibly indicating a region of more recent, although subdued, star formation activity. There is no apparent spiral structure or distinct disk. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal disruptions, although a minor disturbance cannot be entirely ruled out due to the faintness of the outer regions. The shape is approximately round.
