The galaxy presents a largely smooth and centrally concentrated morphology.  The light profile appears relatively featureless with a slightly elliptical shape. The central region exhibits a yellowish-white hue, suggesting an older stellar population. The outer regions transition to a slightly bluer color, indicating the presence of some younger stars. No prominent spiral arm structures or distinct dust lanes are readily discernible in the image, nor are there obvious signs of tidal disturbances or ongoing mergers. It seems to be an intermediately sized galaxy.
