The galaxy presents a generally smooth, elliptical morphology. Its color appears yellowish-white, suggesting a population of older stars, though there may be some ongoing star formation activity present. The overall shape is relatively round, with a slight elongation along a discernible axis. The light is concentrated towards the center, indicating the presence of a central bulge and the luminosity decreases gradually outwards from the core. There are no distinct spiral arms or bar structures visible, and no signs of any major merger events or tidal distortions. The galaxy exhibits a high degree of symmetry.
