This galaxy presents as a relatively smooth, elliptical form, appearing somewhat oblate rather than perfectly spherical. There is a concentration of light towards the central region, suggesting a prominent galactic nucleus. The color gradient transitions from a yellowish-white core to a slightly bluer outer halo. There's minimal evidence of spiral arm structure or significant dust lanes. The galaxy appears to be isolated, without any clear signs of ongoing major merging activity, though subtle disturbances cannot be ruled out. The overall morphology points towards a relatively evolved system, consistent with a large stellar mass and moderate star formation rate.
