The galaxy exhibits a generally smooth morphology, with a high degree of central concentration. It appears elliptical, exhibiting a slightly elongated shape. The core of the galaxy presents a bright, yellowish-orange hue, indicating a high concentration of older stellar populations. The outer regions display a gradual decrease in luminosity, shifting toward a bluer color, which might suggest the presence of younger stars, or star forming regions in the outer regions. There is no clear evidence of strong spiral arms, bars, or tidal features. The galaxy appears relatively undisturbed, lacking any significant signs of recent or ongoing major mergers. There is no prominent dust lane visible. Overall, the galaxy presents a consistent and integrated structure, typical of an early-type galaxy.
