The galaxy presents as a relatively smooth and concentrated object. The central region exhibits a bright, yellowish-white glow, suggesting a significant population of older stars. Moving outward from the center, the light becomes more diffuse and slightly redder in hue. The overall shape appears somewhat elliptical, though not perfectly circular. There is very faint indication of a possible disk-like structure, though it is largely obscured by the dominant central bulge. Overall, the galaxy's morphology suggests an evolved system with low current star formation. There are possible indications of minor disturbance in the form of some asymmetry in the outer regions but it is hard to distinguish.
