The galaxy presents as a somewhat elliptical structure, with a smooth, diffuse appearance. The central region is characterized by a higher surface brightness, exhibiting a yellow-orange hue, suggestive of an older stellar population. The outer regions are less defined and bluer, potentially indicating a population of younger stars or regions of active star formation, although this activity appears subdued. There is a slight asymmetry to the galaxy's shape; it is not perfectly elliptical, hinting at a possible past interaction or internal dynamical process. There is no obvious dust lane or prominent spiral arm structure visible. Overall, the galaxy appears relatively undisturbed, showing only subtle morphological features beyond its basic elliptical form.
