The galaxy presents a morphology indicative of an ongoing or recent merger event. The light distribution reveals a centrally concentrated, smooth component, but with notable asymmetry. There appears to be a second concentration of light, somewhat separated from the primary nucleus. This second concentration could represent the core of the merging galaxy. Tidal features such as faint bridges or tails appear to be absent in this image; therefore, this suggests a system which is smooth, but potentially undergoing a minor interaction. The main body of the galaxy displays a yellow/red color, which may imply an older stellar population. The galaxy exhibits a round shape with slight disturbances. A definitive classification is difficult from the image alone.