The galaxy presents a generally elliptical morphology, appearing largely smooth and spheroidal in structure. A central, bright bulge region dominates the galaxy's luminosity profile. The color of the galaxy appears yellowish-orange, potentially indicating an older stellar population with relatively low ongoing star formation. There may be faint hints of a disk component subtly embedded within the spheroidal structure, as suggested by a slight elongation. However, the overall impression is that of a relatively evolved system with a high degree of radial symmetry. There is no clear evidence of significant tidal interactions or major disturbances in its morphology. The galaxy is compact with a light halo surrounding it. 
