The galaxy presents as a somewhat elliptical, face-on system. The central bulge exhibits a bright, concentrated luminosity, suggesting a high stellar density, and it has an ochre color profile. The color suggests a population of older stars. Surrounding this core is a more diffuse, less luminous disk. The disk seems to be moderately smooth and featureless, lacking prominent spiral arm structures or distinct dust lanes. The color in the outer regions appears slightly bluer than the central bulge, indicating the presence of a younger stellar population. Overall, this galaxy appears to be a relatively evolved system, possibly an early-type spiral or a lenticular galaxy, exhibiting ongoing, but relatively low, star formation. There is no evidence of major merger activity or significant tidal disturbances in the visible structure.
