The galaxy presents as a concentrated, elliptical-like structure with a smooth, diffused light distribution. The central region exhibits a high luminosity, with colors trending toward the redder end of the spectrum, indicative of an older stellar population. The outer regions gradually fade into the background, showing no distinct spiral arms or significant dust lanes. The overall morphology suggests a relatively evolved system, potentially undergoing or having completed its transition from a more active, star-forming phase. There is very little evidence of recent mergers or major disturbances, although subtle asymmetries in the light distribution cannot be entirely ruled out given the image resolution. Overall, it appears to be a quiescent system with a substantial mass, that has undergone substantial evolution.
