The galaxy presents as a concentrated, centrally-brightened object, approximately circular in appearance. Its core exhibits a yellowish-white hue, suggestive of an older stellar population. Moving outwards from the core, the light becomes less concentrated and more diffuse, fading into the background sky. The outer regions display a bluer tint, hinting at the presence of younger, hotter stars, even though these features are hard to discern from the background. There may be subtle signs of weak spiral arms or perhaps a disk structure, although these are not well defined. Faint tidal features or disturbances may be present but are inconclusive from the current image. The galaxy does not appear to be undergoing a major merger, although minor disturbances cannot be ruled out completely. Overall, the galaxy seems to be of moderate mass and relatively quiescent star formation.
