The galaxy presents as a slightly elongated, lenticular shape with a relatively smooth, centralized luminosity profile. The central region exhibits a yellowish-white hue, suggesting a concentration of older stellar populations. Progressing outwards, the galaxy displays a subtle transition to a bluer color, possibly indicative of younger stars. The shape and color distribution suggest an elliptical galaxy exhibiting limited star formation. The lack of well-defined spiral arms and a generally smooth appearance point toward a dynamically relaxed system. There is no evident sign of recent major merger activity, although there are indications of minor perturbations in its structure, but not enough to indicate that the galaxy is actively merging. 
