The galaxy presents as a relatively smooth, centrally concentrated object with a dominant elliptical morphology. It exhibits a bright, ochre-toned core, suggesting a high concentration of older stellar populations. The color profile becomes slightly bluer with increasing radial distance from the center, hinting at the presence of younger stars in the outer regions. There is no obvious spiral structure or prominent dust lanes visible. Faint, irregular features or minor disturbances are potentially present in the outer halo, though the image resolution limits definitive characterization. Overall, the galaxy appears to be a massive system, undergoing low levels of star formation, and generally relaxed, with hints of past minor interactions.
