The galaxy presents as a largely smooth, spheroidal object. There is a concentration of light towards the center, suggesting a central bulge or core. Color gradients are subtle but appear to transition from a warmer, yellowish-red hue in the center to a slightly cooler, greenish-blue tinge in the outer regions. This color variation could indicate differences in stellar populations or dust content. A very slight asymmetry may be present, although the overall morphology appears quite regular and undisturbed. There is no clear evidence of spiral arms, bars, or any significant tidal features indicating recent merger activity. The galaxy's light is relatively well-defined, without a significant diffuse halo extending far beyond the main body.
