The galaxy presents a morphology that appears to be intermediate between smooth and disk-like. The light distribution indicates a central bulge of considerable brightness, with a color profile tending toward redder hues. Extending from this bulge is what appears to be a fainter, less-defined structure, possibly a disk component. There is evidence of disruption or irregular features possibly caused by gravitational interactions. The galaxy exhibits hints of disturbances, potentially suggesting an ongoing or recent merging event. The overall form could be classified as an elliptical galaxy with possible tidal features, or a spiral galaxy undergoing disruption.
