The galaxy presents a generally smooth morphology, appearing largely featureless with a high degree of central concentration. The shape is elongated, tending towards a spheroid rather than a flattened disk. There is a hint of asymmetry to the outer isophotes, suggesting a possible tidal interaction or minor disturbance. Color gradients indicate a central region that is yellower, potentially indicating an older stellar population, while the bluer colors in the outer reaches suggest ongoing, but weak, star formation in some areas. There is no clear spiral structure or bar feature visible. Evidence suggests it is a fairly massive galaxy.
