The galaxy presents as a somewhat elliptical, disk-like structure with a prominent central bulge. The bulge exhibits a yellowish-white hue, suggesting a population of older stars. Surrounding the bulge is a bluer disk, likely indicative of ongoing star formation. The disk appears relatively smooth with some subtle hints of spiral arm structures. The overall color gradient transitions from a warmer core to cooler, bluer outer regions. The galaxy does not appear to be strongly disturbed, but there are hints of faint tidal features or asymmetries, potentially suggesting past interactions or ongoing minor disturbances. The galaxy's light profile is relatively smooth, hinting at a Sersic index in the range of typical spiral to elliptical galaxies.
