The galaxy appears as a single, elliptical-like object with a smooth, diffuse light profile. The central region exhibits a concentrated brightness, suggesting a higher density of stars. The color is generally yellow-orange, indicating an older stellar population with lower star formation rates and the likely presence of evolved stars. There is a small secondary object, possibly another galaxy, that may be merging. The system appears to be undergoing some kind of gravitational interaction. There are no distinct spiral arms or dust lanes visible.
