This galaxy exhibits a generally elliptical morphology, with a smooth, concentrated central bulge dominating its overall appearance. The light profile suggests a relatively uniform distribution of stars, without prominent spiral arm structures or distinct knots of star formation readily visible. Its color is moderately red-shifted, indicating a population of older stars with lower rates of on-going star formation. There is no clear evidence of any active galactic nuclei or significant dust lanes. The galaxy appears relatively undisturbed, showing no signs of recent or ongoing merger activity. Based on its physical size, the galaxy is fairly massive, potentially containing over one hundred billion stars.
