The galaxy presents an overall elliptical morphology, appearing generally smooth and relatively featureless. There is a central concentration of light, suggesting a bulge component. The color profile shifts from a yellowish-white core to a bluer halo region, implying a mix of stellar populations, with older stars concentrated towards the center and younger, bluer stars distributed more peripherally. The galaxy exhibits an intermediate apparent roundness, not perfectly spherical but not highly elongated either. There is no visible evidence of ongoing major mergers or strong tidal disturbances, although a subtle asymmetry in the outer regions could suggest minor interaction or internal dynamical processes.
