The galaxy presents as an elliptical-like system. It exhibits a smooth, centrally concentrated light profile with a slight elongation. The major axis appears oriented at approximately 25 degrees from the horizontal. The light distribution appears to be relatively uniform across the galaxy with the exception of a very bright central core. There are some color gradients apparent within the system. The central region has a yellowish-white hue, suggesting an older stellar population. The outer regions appear slightly redder. There is no discernible spiral arm structure or dust lanes visible. The galaxy appears relatively undisturbed, showing no strong evidence of recent merger activity.
