The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. The core exhibits a bright, yellowish hue, indicative of an older stellar population. There is no discernible dust lane or spiral arm structure. The galaxy appears to be relatively isolated, showing no signs of major interaction or merging. The outskirts of the galaxy appear somewhat diffuse and less luminous, fading into the background sky. Overall, the galaxy seems to be a relatively undisturbed, evolved system.
