The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. The core exhibits a bright, yellowish-white hue, indicative of a population of older stars. Moving outward from the core, the light gradually diminishes, transitioning to a reddish-orange color. There are hints of asymmetry, with a slight elongation along one axis, but no distinct spiral arms or bar structures are discernible. The galaxy appears to be fairly isolated, with no obvious signs of major interaction or recent merger activity. Based on the colors, it may be a relatively massive galaxy with low star formation rates.
