The galaxy presents as a relatively smooth, centrally concentrated elliptical morphology. Its overall color profile suggests an older stellar population, with a yellowish-orange hue dominating the galactic body. There is a subtle fading of luminosity from the core outwards to the edges, indicating a decreasing density of stars. The galaxy exhibits a moderate degree of roundness, with a slight deviation from a perfectly circular shape. No prominent spiral arms or significant dust lanes are discernible. Possible minor tidal disturbances may be influencing the outer regions, but these features are not definitive. Overall, this galaxy appears to be a massive, quiescent system with a low rate of star formation.
