The galaxy presents as a relatively smooth, elliptical morphology. Its core exhibits a bright, concentrated luminosity, suggestive of an older stellar population. The galaxy appears primarily featureless, with a high degree of symmetry. There's an apparent lack of strong dust lanes or spiral arm structures. A slight elongation is observed, deviating from a perfect circular shape, leaning towards an in-between roundedness. No major mergers are observable, but there could be minor disturbances present. The color profile indicates a moderate age, with light from younger stars still contributing. The overall appearance aligns with an early-type galaxy that is not currently undergoing intense star formation activity.
