The galaxy presents a generally smooth morphology, with a high degree of central concentration. The shape is elongated and appears intermediate between round and cigar-shaped. It is dominated by a significant bulge that exhibits a yellowish-orange hue, suggesting a population of older stars. Fainter blue color in the surrounding galactic disk suggests the presence of some younger stars. The galaxy does not appear to be undergoing any major mergers, although there is a slight hint of disturbance in the outer regions.
