The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and rounded morphology. The central bulge region is bright and concentrated, showing a high degree of symmetry. There is little evidence of spiral arm structures or prominent dust lanes. The galaxy appears to be relatively undisturbed, without any significant tidal features or signs of an ongoing major merger. Some slight color variations are visible, with the central region appearing bluer than the outer regions, which appear more red. This may indicate some ongoing, though likely minimal, star formation activity in the core. Overall, this galaxy seems to be a well-formed, evolved system nearing the end of it's star forming lifecycle.
