The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, with a high degree of roundness. There is little discernible substructure or distinct features within the galaxy's light profile. Faint color gradients appear, with the central region exhibiting a slightly bluer hue compared to the more extended, redder outer regions. There is no obvious evidence of any significant ongoing merging activity or major disturbances to the overall galactic structure. A slight asymmetry can be observed, although the cause of this is not obvious, but is likely a minor interaction. It's quite compact in apparent size.
