The galaxy presents as a somewhat diffuse, oblong structure with a notable central bulge. The central region exhibits a smoother texture and a brighter, more concentrated luminosity. The surrounding disk appears to be more irregular, showing hints of faint spiral arms or tidal disturbances. Overall, the galaxy appears to be in an intermediate stage, possibly transitioning between a spiral and an elliptical morphology. There is a slight asymmetry, suggesting a potential interaction or merger history. Some subtle color variations are present, with bluer regions possibly indicating areas of recent star formation.
