The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular classification. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. While generally smooth, a faint indication of a disk-like structure or some other features are present within it. Its shape is somewhere in between round and cigar shaped, more leaning towards an elliptical shape. There is no apparent sign of an ongoing major merger, tidal tails, or strong gravitational disturbances. The color indices indicate a population of older stars, consistent with a relatively low star formation rate.
