The galaxy presents as a relatively smooth, centralized structure. It appears elliptical, with a dominant, round morphology. A slight elongation is perceptible, but the galaxy leans towards a circular appearance.

The color distribution suggests a concentration of older stellar populations in the central region, indicated by the reddish hue. A subtle, less-concentrated presence of younger stars are present. There are no signs of strong tidal features. It does not appear to be undergoing a major merger or significant disruptive event. The galaxy displays characteristics of a quiescent system with ongoing, albeit mild, star formation.
