The galaxy presents a generally elliptical morphology. The central region exhibits a high surface brightness, appearing almost uniformly bright with a yellowish hue, suggesting an older stellar population. The outer regions fade gradually, exhibiting a slight ellipticity. The color becomes marginally bluer in these extended areas, hinting at the presence of some younger stars or ongoing, albeit low-level, star formation. There is no evidence of strong spiral arm structure or distinct dust lanes visible in this image, and the galaxy appears relatively undisturbed. The general smoothness and lack of prominent features suggest it is likely a relatively evolved system.
