The galaxy presents a predominantly smooth, elliptical morphology, with a diffuse, concentrated bulge. There is minimal evidence of spiral arms or a disk structure, suggesting a more evolved system. The galaxy's overall color appears relatively homogenous, with slight variations indicating differing stellar populations or dust distribution. The galaxy exhibits a round, well-defined shape, lacking significant tidal disturbances or signs of interaction with other galaxies, but a slight asymmetry could be present. It is likely a large galaxy, based on the overall brightness. The light distribution suggests minimal ongoing star formation activity. A possible minor merger is not ruled out, but the system appears to be largely isolated and relaxed.