The galaxy presents a predominantly smooth, elliptical morphology, exhibiting a generally round shape with slight elongation. The central region appears brighter and yellowish in color, likely indicating a concentration of older stellar populations. Fainter, diffuse extensions emanate from the core, suggesting a gradual decline in stellar density with increasing radius. Subtle color gradients are observed, with the outer regions potentially exhibiting a bluer hue compared to the core. There is little evidence of spiral arm structure or significant dust lanes. The galaxy appears relatively undisturbed, without pronounced tidal features or signs of ongoing major merger activity, though subtle disturbances cannot be ruled out. Overall, the galaxy appears to be a relatively evolved system, potentially in the process of quenching star formation.
