The galaxy presents as a relatively smooth, centrally concentrated object with a somewhat elliptical morphology. The light profile appears diffuse with a gradual decline in intensity from the center outwards. The central region exhibits a bright, concentrated core, likely indicating a higher stellar density or possible active galactic nucleus. There is a slight elongation visible, suggesting a mild deviation from a perfect spherical shape. The overall color appears blue-white, hinting at a population of younger, hotter stars and ongoing star formation, though it is mostly considered smooth. There is no apparent spiral structure or distinct dust lanes visible in this image; however, there may be the appearance of a very slight merging event. The galaxy appears fairly isolated, with no immediately apparent tidal features or interacting companions.
