The galaxy presents as a somewhat flattened, elliptical morphology. It exhibits a concentrated central bulge, emitting a bright, relatively uniform light. The light gradually decreases in intensity from the core outwards, suggesting a diminishing stellar density. The overall color profile appears to be slightly bluer towards the center, becoming redder in the outer regions. There is no evidence of prominent spiral arms or distinct dust lanes. The outer regions of the galaxy gradually fade into the background, appearing smooth with no obvious signs of tidal disturbances or interactions.