The galaxy presents as a centrally concentrated object, exhibiting a relatively smooth morphology. The light profile appears to decrease gradually from the core to the outer regions with no obvious spiral arms. A slight ellipticity can be observed in its overall shape, which is neither perfectly spherical nor highly elongated. The color gradient suggests a concentration of older stellar populations in the core, which transitions to slightly bluer colors in the outer regions, perhaps indicating more recent star formation activity at the edges. No significant signs of tidal disturbances, or other indications of a recent major merger event are evident. Minor asymmetries in the outer halo suggest the possibility of past minor interactions.
