The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears to be elliptical or spheroidal, with no immediately obvious spiral arm structures or a prominent disk component. The light profile suggests a high degree of central concentration, with luminosity decreasing gradually from the core outward. The color appears generally yellow/gold, indicating an older stellar population. There is no evidence of active galactic nuclei activity nor recent major mergers. There are no distinct tidal features or strong morphological peculiarities, suggesting it has not undergone any recent major interaction. It appears to be an isolated, well-formed system.