The galaxy presents as a single, relatively smooth structure with a concentrated central bulge. It appears largely elliptical in shape, though possibly with a slight distortion. The color is predominantly yellow-orange, suggesting an older stellar population with a lower rate of recent star formation. There is no evidence of spiral arms or prominent dust lanes. The light is fairly concentrated, with a gradual decrease in brightness moving outwards from the core. There might be some minor asymmetry in the outer regions, potentially indicating past or ongoing interactions, but this is not definitive from the image alone. Overall, the galaxy appears as a passively evolving system.
