The galaxy appears as a diffuse, centrally concentrated object, showing characteristics of both a smooth morphology and disk-like features. The central region is brighter and more condensed, suggesting a significant concentration of stars and potentially a bulge component. The outer regions exhibit a less defined structure, with a hint of a flattened disk or spiral arm segments, though their form is irregular and undefined. The overall shape is somewhat elliptical, but deviates from a perfect ellipse, indicating possible tidal disturbances or recent interactions. Colors are somewhat blue-shifted, indicating a younger stellar population and potential ongoing star formation. There are also hints of potential merger activity, possibly minor disturbances or interactions with another galaxy.
