The galaxy presents as a centrally concentrated object with a smooth, somewhat elliptical morphology. The core exhibits a bright, yellowish-white luminosity, suggesting a concentration of older stellar populations. There's a gradual decrease in surface brightness moving outward from the core, with a faint, diffuse halo extending beyond the brighter central region. No distinct spiral arms or prominent dust lanes are visible. The overall color is consistent with an older stellar population and minimal on-going star formation. Subtle irregularities in the outer regions might indicate minor gravitational interactions, but the galaxy appears largely undisturbed.
