The galaxy presents as an elliptical morphology, with a smooth, concentrated luminosity profile. It appears largely featureless, lacking prominent spiral arms or distinct dust lanes. The color indices suggest a relatively evolved stellar population. There is a slight elongation noticeable in the shape, though it leans towards a rounded appearance. There is no apparent evidence of on-going major merging activity, though a minor disturbance cannot be ruled out based on the galaxy's asymmetry. There is a hint of possible tidal features or disturbances, but image clarity limitations prevent a definitive assessment.
