The galaxy presents as a largely smooth structure, likely an elliptical or lenticular type. The central region exhibits a high concentration of light, suggesting a dense stellar population and possibly a supermassive black hole at the core. The overall shape is roughly elliptical, displaying a moderate degree of roundness with subtle deviations from a perfect circle. There is faint indication of a disturbance or tidal feature suggesting some kind of galactic interaction in the recent past. Overall, the galaxy appears to be undergoing some form of evolution.
