The galaxy presents as a relatively smooth, elliptical-like structure, with no apparent spiral arms or significant dust lanes visible at this resolution. There is a high concentration of light towards the center, suggesting a prominent bulge. The color profile appears generally redder, particularly towards the core, indicative of an older stellar population. The overall shape indicates it is an elliptical galaxy with a medium size and a moderate redshift, indicating it is at a considerable distance from our own. There are no other notable interactions or features in the immediate vicinity, such as tidal tails or obvious signs of an ongoing merger.
