The galaxy presents a generally smooth appearance, suggesting a relatively evolved system. Its shape appears to be somewhere between round and elongated. There is subtle asymmetry present, potentially indicating a minor gravitational interaction or internal disturbance. The galaxy exhibits a color gradient, appearing slightly bluer in its central region and trending redder towards the outer edges, suggestive of on-going, though potentially low, star formation activity within its core. There are no obvious spiral arm structures or prominent dust lanes visible, implying it is likely an elliptical or lenticular galaxy. Faint tidal features might be present, but these are difficult to discern definitively. The system appears to be relatively massive with moderate to high star formation rates for an object of this type, contributing to its high luminosity across the observed g, r, and z bands.
