This galaxy exhibits a primarily smooth morphology, with a subtle disk-like structure hinted at in its overall shape. The central region appears as a bright, elliptical core, potentially indicative of an older stellar population. A ring of bluer light surrounds the core, possibly indicating a region of active star formation. There may be a minor disturbance of tidal stream visible in the bottom right of the image. The main body shows no obvious signs of major mergers or significant tidal disruptions. The galaxy appears as an isolated system.
