The galaxy appears as a moderately bright, somewhat elongated object. It exhibits a central concentration of light that fades gradually towards the edges. There's evidence of a disk structure, although it is not sharply defined. The galaxy's color appears to be a mix of yellow-orange in the core, possibly indicating an older stellar population, with hints of bluer hues in the outer regions, perhaps suggesting more recent star formation. Some asymmetry might be present, and there do not appear to be any major disturbances or mergers. Overall, the galaxy presents a relatively smooth and integrated appearance.
