The galaxy presents as a relatively smooth, elliptical-like structure. There is a central, bright core region that gradually fades outwards. The color profile suggests a redder overall hue. The galaxy appears to be moderately compact, with no significant visible signs of spiral arms or major disturbances from galactic mergers. It exhibits a high degree of central concentration, with light dropping off rapidly from the core to the outer regions. The overall morphology points toward an older stellar population with little ongoing star formation. The galaxy appears to be isolated, without any close companions or interactions.
