The galaxy presents as a centrally concentrated spheroid with a smooth, largely featureless morphology, suggesting it is an elliptical galaxy. A diffuse, extended halo surrounds the central bulge, fading gradually into the background sky. The light distribution exhibits a slight elongation, deviating marginally from a perfectly circular shape. There are subtle color gradients, with a slightly redder hue towards the center, potentially indicating a higher concentration of older stellar populations. Faint disturbances or minor distortions are possibly present in the outer regions, implying past or ongoing interactions with other galaxies. The overall impression is of a mature, relatively quiescent system, though subtle signs of activity exist.
