The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a high degree of radial symmetry with a dominant central bulge. There is minimal evidence of a distinct disk component, or spiral arm features. The color profile suggests an older stellar population. The light distribution appears centrally concentrated, with a gradual decline in luminosity moving outward from the core. There are no prominent dust lanes visible and no signs of major ongoing mergers. The galaxy displays a somewhat concentrated shape.
