The galaxy appears as an elliptical structure with a generally smooth morphology. The core region exhibits a concentration of light, transitioning gradually into the outer regions. There appears to be minimal dust obscuration, the galaxy is of an intermediate size. The object displays no prominent spiral arms or other distinct features. The color gradient suggests a potentially evolved stellar population. No obvious signs of tidal interactions or ongoing mergers are visible in the immediate vicinity. Overall, the galaxy seems relatively isolated.
