The galaxy presents a largely smooth, elliptical morphology. Its color profile suggests a dominant population of older stars, indicated by the yellowish hue concentrated toward the central bulge. Hints of bluer colors are present in the outer regions, implying the presence of some younger stellar populations, although they are not very distinct. There is a slight asymmetry or minor distortion present, although its origin is not readily apparent. It could suggest a minor interaction or internal dynamics. Overall, the galaxy appears to be a massive system with reduced star formation activity, though not entirely quiescent.
