The galaxy presents as a centrally concentrated, largely smooth structure. There is a pronounced elliptical morphology, appearing nearly circular. The light distribution shows a radial gradient, brightest at the core and diminishing outwards, suggestive of an older stellar population in the central region. There is some indication of a possible faint disk, however the limited resolution makes a detailed morphological classification difficult. Subtle color variations are observed, with a slightly bluer tinge on the edges suggesting the potential of faint recent star formation activity in the outskirts of the object. The galaxy appears relatively undisturbed.
