The galaxy presents as a centrally concentrated elliptical with an overall smooth morphology. The core exhibits a bright, intense yellowish-white luminosity, suggesting a high concentration of older stars. The outer regions display a gradual decrease in surface brightness, fading into the background sky. The overall color is consistent with a population of older, less massive stars, indicating a relatively low star formation rate. There is no discernable spiral arm structure or prominent dust lanes. The shape appears moderately elliptical, not perfectly spherical. The smooth appearance dominates, with no signs of significant disturbances or ongoing mergers visible in the image.
