The galaxy presents as a luminous, elliptical morphology with a notable central bulge. The overall color profile appears somewhat redder, indicative of an older stellar population and reduced recent star formation activity. A subtle disk-like structure may be present, though it's difficult to discern due to the galaxy's predominantly smooth appearance. There might be faint dust lanes or other features within the galaxy. The galaxy appears relatively undisturbed, suggesting it is not currently undergoing a major merger event.
