The galaxy presents as a relatively smooth, elliptical structure. The central region displays a bright, concentrated luminosity, suggestive of a dense stellar population or possible active galactic nucleus. There are no readily apparent spiral arms or distinct disk-like features. The galaxy appears slightly elongated but overall lacks major distortions that would indicate a recent or ongoing major merger event. The color profile exhibits a slight gradient, transitioning from a bluer hue in the core region to a redder color in the outer regions. It appears relatively isolated with no immediately obvious interacting companions.
