The galaxy presents as a fairly smooth, centralized structure, appearing elliptical or lenticular in form. It exhibits a notable color gradient, transitioning from a yellowish core to a slightly bluer outer region, suggesting a mix of older stellar populations in the center and possibly younger, star-forming regions in the outer disk. No spiral arm structures are readily apparent. The galaxy’s shape is mostly round, with a faint disturbance on one end that may imply minor tidal interactions or internal asymmetries. Overall, the light distribution indicates a relatively mature galaxy with moderate levels of on-going star formation.
