The galaxy appears to be a relatively bright, isolated system. It exhibits a centrally concentrated morphology, with a bright, well-defined core that decreases in intensity outward. The overall shape is somewhat elliptical, leaning towards a more rounded appearance. There is evidence of a disk component, but it is not sharply defined, appearing more as a gradual fading of the central light. The galaxy's color is a pale blue-white, which suggests a relatively old stellar population, with moderate levels of ongoing star formation. There is no strong indication of any major tidal disturbances or mergers, but subtle irregularities in the outer regions could indicate minor interactions or past events.
