The galaxy appears to be an elliptical type. It presents a centrally concentrated luminosity profile with a smooth appearance. The central region displays a brighter concentration of light, gradually decreasing towards the outer edges. The galaxy's overall shape is moderately elliptical, trending towards an intermediate spheroidal form rather than a highly flattened disk or elongated cigar shape. There appears to be evidence of a potential ongoing or recent merger event. One tidal tail is visible, suggesting a relatively undisturbed system, but is likely the result of ongoing accretion or a minor interaction. The system has moderate star formation, and is likely a massive galaxy. 
