The galaxy presents as a single, relatively smooth and centralized object, with a slight elongation along its primary axis. It exhibits a color gradient, transitioning from a yellowish-white core to a bluer periphery. The central region appears to dominate the overall light emission. A faint disk-like structure can be inferred, but detailed morphological features are not readily discernible. The overall structure suggests a possible ongoing or past minor disturbance that has not dramatically disrupted the system. There may be a slight asymmetry in the outer regions of the galaxy, hinting at potential interaction or recent accretion event. The overall color profile indicates a moderate redshift.
