The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a strong, concentrated luminosity, suggesting a high density of stars. The light distribution falls off gradually from the center outwards. There is no observable spiral arm structure or distinct dust lane. The color appears to be a reddish-yellow hue. Based on the color and morphology, this is likely a relatively quiescent galaxy with minimal ongoing star formation and a significant population of older stars. There may be slight asymmetries in its halo. There is no clear evidence of a major ongoing merger.
