The galaxy appears as a relatively smooth, elliptical structure with a dominant central bulge. There is a subtle color gradient, transitioning from a yellowish hue at the core to a slightly redder tinge in the outer regions. The overall shape is neither perfectly spherical nor significantly elongated, leaning towards an intermediate classification.

There is no apparent spiral arm structure or significant dust lane obscuration visible. The galaxy's light profile suggests a moderate degree of concentration around the nucleus. It exhibits a relatively quiescent morphology, with no obvious signs of ongoing major merger activity. However, a slight asymmetry in its outer halo could indicate a past interaction or minor disturbance. 

Based on its overall color and morphology, the galaxy is likely composed predominantly of an older stellar population, with a relatively low current star formation rate. The galaxy is of moderate size, spanning an estimated diameter of roughly 9 kpc.
