The galaxy presents as a single, concentrated object with a relatively smooth appearance. The central region exhibits a higher surface brightness, indicative of a dense stellar population and possibly a supermassive black hole at its core. The overall color appears yellowish, suggesting an older stellar population with fewer young, massive stars. The morphology indicates a high probability of merger activity, with a non-negligible possibility of a major disturbance being present in the structure, even though it mostly appears to be smooth. The relatively high mass estimates and low star formation rate suggest that the galaxy might have consumed most of its star-forming gas in the past and may now be evolving passively. The galaxy has an angular size consistent with its physical size, as determined by its estimated distance.
