The galaxy presents a predominantly smooth morphology, suggesting characteristics of an elliptical galaxy or a lenticular galaxy viewed face-on. The light distribution shows a strong central concentration, becoming less dense towards the outer regions, this implies a dominant bulge component. The shape is neither perfectly spherical nor highly elongated; a slightly ovoid structure is observed, which is supported by the intermediate roundness. Faint hints of a disk structure are discernible but are not dominant. There are some disturbances in the galaxy in the form of asymmetry, but not in a highly merging or violently interacting state. It shows a relatively low rate of star formation. The color of the galaxy exhibits a redder hue, indicating an older stellar population.
