The object presents as a singular, relatively symmetrical galaxy at a considerable distance. The morphology appears to be primarily smooth with a notable lack of defined spiral arms. It exhibits a slightly elliptical shape, leaning towards rounded rather than elongated. The galaxy's core region displays a higher concentration of light, gradually diminishing towards the outer edges. The color profile suggests a mature stellar population, with a noticeable presence of older, redder stars, though some bluer regions suggest recent star formation. Based on the apparent distortions and irregular shape, it appears likely to be undergoing, or to have recently undergone, a merger event with at least one other galactic object. There is evidence of some tidal disturbances in the outer regions of the galaxy.
