The galaxy presents a largely smooth, elliptical morphology. The central bulge exhibits a bright, concentrated luminosity, suggesting a high density of stars. This light appears yellowish. Fainter, bluer light surrounds this central region, implying the presence of a stellar disk. The object appears largely undisturbed, with no obvious signs of major mergers or tidal interactions. There is the possibility of a minor disturbance or possible interaction in the form of a small, faint object close to the main galaxy. The galaxy's color index suggests that it is mostly composed of older stars, but still has some younger stars. The absence of strong spiral arm features or prominent dust lanes supports its classification as a galaxy with a significant spheroidal component. Overall, the galaxy appears to be a relatively evolved system, exhibiting characteristics of a galaxy near the transition from star-forming to quiescent.
