The galaxy presents a generally smooth morphology, appearing largely featureless. Its shape is somewhat round, though there is a slight deviation from perfect circularity. There are subtle irregularities in the galaxy's structure. There is no strong evidence of a major ongoing merger, although there are hints of minor disturbances or tidal features that could be indicative of past interactions. The galaxy exhibits a faint but discernible disk-like component. Based on the observed color indices and the presence of disk features, some ongoing star formation may be present.
