The galaxy presents as a somewhat elongated, smooth object, appearing mostly featureless in this image. It exhibits a bright central region, indicating a concentration of stars and possibly an active galactic nucleus, though this cannot be definitively determined from the image alone. The galaxy shows a distinct color gradient, shifting from a bluer hue in its core to redder tones toward the edges, which may be indicative of a differential stellar population. A higher degree of red-shifted light in the outer regions suggests older stellar populations. There are also hints of a minor dust lane or other structural irregularity near the core. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions.
