The galaxy presents a largely smooth, elliptical morphology. It appears approximately round in shape, with a slight deviation towards an intermediate form. The light distribution is concentrated towards the center, exhibiting a prominent bulge. No distinct spiral arm structures or bar features are visible. There are hints of minor disturbance, such as faint asymmetries or slight distortions in the outer regions, though the overall structure is largely undisturbed. The color indices suggest the presence of a population of older, redder stars, indicative of a relatively quiescent star formation history. The estimated size corresponds to a galaxy of substantial extent.
