The galaxy appears as a relatively smooth, elongated structure with a noticeable central bulge. The color gradient suggests a composition of older stellar populations dominating the core, with possibly younger, bluer stars present in a fainter disk or extended halo. There is no strong evidence of significant spiral arm structure or active star formation regions visible in this image. The galaxy's shape is somewhat oblate, appearing more rounded than highly elongated. The overall impression is that of an evolved galaxy, possibly an elliptical or lenticular galaxy, with minimal signs of ongoing mergers or major disturbances. The absence of prominent dust lanes also supports the characterization of an older, less actively star-forming system.
