The galaxy presents a largely smooth morphology, with a high degree of central concentration. The overall shape appears somewhat elliptical, though not perfectly circular; it exhibits a slight elongation. The color profile suggests an older stellar population, given the redder hue of the central bulge, and the lower mass suggests star formation has slowed in this galaxy. There is some visual evidence of a slight tidal disturbance, but the galaxy appears largely undisturbed. There is no clear evidence of strong spiral arm structures or a distinct disk component.
