The galaxy presents as a centrally concentrated object, exhibiting a spheroidal morphology. A smooth, diffuse light profile characterizes the main body, with a gradual decline in luminosity from the core outwards. The core appears to be an active region with high luminosity. There is a faint disk extending from the center of the galaxy. The galaxy lacks any distinct spiral arm structures. It exhibits a yellow-white hue, indicative of a stellar population that is relatively old and with low star formation activity. There is no evidence of recent major merger events or significant tidal disturbances. The overall appearance suggests a relatively quiescent system, possibly a mature elliptical galaxy.
