The galaxy presents a generally smooth appearance. The color profile suggests an older stellar population, with a concentration of light in the redder wavelengths. The object is elliptical in shape, exhibiting an intermediate roundness that deviates minimally from a perfect circle. There is no visually significant evidence of active merging or major disturbances, though minor disturbances cannot be ruled out. Based on the color and morphology, this galaxy is likely a quiescent galaxy with a dominant spheroidal component.
