This galaxy presents as a relatively compact, elliptical-like structure. The central region exhibits a bright, concentrated core, suggesting a higher density of stars and potentially a supermassive black hole at its center. The luminosity decreases gradually moving outward from the core.

The overall color of the galaxy appears yellowish-white. The color suggests an older stellar population dominated by evolved stars, with minimal ongoing star formation. There may be subtle color gradients visible, with the central region appearing slightly more yellow than the outer regions.

While there is some indication of a faint disk-like structure, the galaxy's overall form lacks well-defined spiral arms or other distinct features commonly associated with spiral galaxies. There is a slight asymmetry in the shape of the outer regions, which could indicate a past interaction or merger event, although there are no clear signs of tidal tails or other significant disturbances.
