The galaxy presents a generally elliptical morphology, though deviations from a perfectly smooth profile are present. The central region exhibits a bright, concentrated nucleus with a high surface brightness, suggesting the presence of a significant stellar population or active galactic nucleus. The overall color profile appears slightly bluer towards the central regions. The outer regions of the galaxy are less defined, with a diffuse, irregular halo extending beyond the main body. There is a faint indication of minor structural asymmetry, hinting at possible gravitational interaction. The galaxy's overall light distribution is suggestive of a system that has undergone or is undergoing some form of disturbance.
