The galaxy presents a generally smooth morphology, with some indication of internal structure. The central bulge is prominent and exhibits a bright, concentrated luminosity. The overall shape of the galaxy appears moderately elliptical. The light distribution suggests an intermediate ellipticity, leaning toward round. There may be a faint disk component present, but it is not sharply defined. There is a possibility of a very minor disturbance present, though this is not definitive from the image. Color gradients are evident; the central bulge displays a redder hue, while the outer regions are relatively bluer.
