The galaxy appears as a centrally concentrated, elliptical structure. It exhibits a smooth, diffuse morphology with no obvious spiral arm features or prominent dust lanes. The core region shows a high degree of luminosity, indicating a dense stellar population, possibly a supermassive black hole at the center. There is a slight elongation visible, but overall, it appears relatively rounded, with most citizen scientists observing it as in between round and elongated. There is little evidence of ongoing or recent major merger events. The galaxy's color gradient suggests an older stellar population. There are some observations of minor disturbances in the galaxy, but the majority of users suggest there is no ongoing major merging events.
