The galaxy presents as a flattened, elongated system. The central region exhibits a diffuse, yellowish-white glow suggesting a population of older stars. Moving outward from the core, there is a noticeable transition to bluer hues, particularly along the longer axis of the galaxy. This color gradient implies the presence of younger, hotter stars forming within these outer regions. The overall structure appears relatively smooth, with no obvious spiral arm structure visible at this resolution. There is some indication of a slight asymmetry or warping to one side of the galaxy, but it is difficult to ascertain whether it is due to internal dynamics or an interaction. The faintness of the outer disk suggests it may be relatively low in stellar density.
