The galaxy presents as an elliptical morphology, with a high degree of central concentration. Its color index suggests the presence of a moderately evolved stellar population. The system appears relatively undisturbed, with no obvious signs of tidal features or ongoing major mergers. The isophotes appear smooth, suggesting little ongoing star formation. There may be some evidence of minor disturbances present. The axial ratio indicates that the galaxy is of intermediate ellipticity, presenting as neither round nor highly elongated. The galaxy has an approximate effective radius of 5 kpc. Its mass is approximately 10^10.8 solar masses. Its star formation rate is 10^-0.6 solar masses per year.
