The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated, bright central bulge. The core exhibits a yellowish-orange hue, indicating a potentially older stellar population. The outer regions of the galaxy appear more diffuse, fading into the background sky. A very faint, disk-like structure may exist, but is not definitively confirmed. No prominent spiral arms or dust lanes are immediately obvious. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal interactions. There are no discernible star-forming regions, suggesting that star formation rate may be relatively low. The galaxy exhibits an intermediate roundness.
