The galaxy appears to be an elliptical galaxy with a smooth, diffuse light distribution and high spheroidal symmetry. The galaxy is slightly elongated, showing deviation from being perfectly round. Color gradients across the galaxy's surface are subtle, with a somewhat redder core transitioning to slightly bluer outer regions. There is no evidence of spiral arms or a prominent disk structure. The overall morphology suggests that this galaxy is likely quite massive, exhibiting a relatively low star formation rate. There are no signs of significant tidal disturbances or ongoing major merger events. Faint hints of asymmetries or minor disturbances might be present, meriting further investigation with deeper imaging data.
