The object presents as a somewhat diffuse, moderately bright galaxy. It appears to be a highly disturbed system. There is evidence of a possible minor merging event or tidal interaction with a companion galaxy, with faint, wispy extensions or streams of stellar material visible in the object's vicinity. A significant fraction of the light appears concentrated in the central region, but this region seems to be irregular, rather than spherical, without a readily apparent nucleus. There may be a distinct but small companion galaxy or a region of intense star formation nearby. The overall morphology suggests a system undergoing a disruptive event, potentially altering its classification as a spiral or elliptical galaxy.
