The galaxy presents as a somewhat flattened, elliptical morphology. The central region exhibits a high surface brightness, appearing a yellowish-white hue, suggesting a population of older stars. The color distribution transitions gradually outward, shifting towards a slightly redder tone. The outer regions appear less defined and fainter, fading into the background sky. The overall smooth appearance suggests a relatively quiescent system with little evidence of active star formation or major disturbances, such as tidal tails or prominent dust lanes. There may be a hint of a slight warp or asymmetry in the disk, but this requires further investigation to confirm.
