The galaxy presents a largely smooth and elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness towards its outer regions. There is a high degree of rotational symmetry, with a near perfect roundness, and it is only very slightly elongated. No distinct spiral arms, bars, or other pronounced features are discernible. There is some evidence of minor disturbances or interactions in the structure. The galaxy's color indices suggest it is composed of an older stellar population, dominated by redder wavelengths. The galaxy's size is estimated to be around 5.37 kpc. Star formation rate is low. The observed redshift indicates it is at a significant distance from us.
