The galaxy presents as a single, relatively featureless object. The central region exhibits a concentrated luminosity, with a color profile suggestive of an older stellar population; the core shows a distinct yellowish-orange hue. The outer regions appear fainter and more diffuse, transitioning to a bluer color, which could be due to a younger stellar population or recent star forming regions in the outer disk. There is a slight asymmetry noticeable in the extended halo, with the upper-left of the galaxy extending slightly further than the other regions. Overall, the galaxy appears to be in a relatively quiescent state with no major ongoing mergers or tidal disturbances readily apparent.
