The galaxy presents as a luminous, relatively symmetrical elliptical or lenticular system. The overall color is a yellowish-white, suggesting a dominant population of older stars. The light distribution appears smooth, with a high degree of central concentration, indicative of an evolved stellar population. No distinct spiral arm structures or prominent dust lanes are discernible. The morphology appears largely undisturbed, showing no significant tidal features or signs of a major merger event. However, there seems to be a smaller, disturbed galaxy or star cluster interacting with the larger one. A possible minor disturbance could be visible as a slight elongation or asymmetry, though it is faint. There is a secondary bluish body that is likely another galaxy, or a star cluster, that may be in a close orbit.