The galaxy presents as an elliptical morphology, appearing largely smooth and relatively featureless. Its shape is moderately elongated, exhibiting an intermediate axis ratio. A bright central bulge dominates the structure, transitioning into a fainter, more diffuse halo. The color gradient suggests a redder core, possibly indicative of an older stellar population concentrated in the center, with slightly bluer regions in the surrounding area potentially suggesting some recent or ongoing star formation. The galaxy does not show any obvious signs of major disturbances or mergers, although there might be hints of minor irregularities in its outer regions.
