The galaxy presents a smooth, elliptical morphology. The central region exhibits a high degree of luminosity, appearing as a concentrated, bright yellowish-white core. Moving outward from the core, the light intensity gradually diminishes, transitioning into a fainter, diffuse halo. The color profile of the outer regions appears slightly bluer compared to the core, suggesting the presence of younger stellar populations within this region. There is no evidence of spiral arms, a central bar, or significant dust lanes. The overall structure suggests a relatively evolved system, likely a massive galaxy with a notable population of older stars, though the presence of some younger stars cannot be ruled out. Minor irregularities in the outer halo could suggest possible minor interactions with smaller galaxies, but without additional data, this cannot be confirmed.
