The galaxy presents a smooth, elongated morphology, appearing cigar-shaped. It exhibits a central bulge that is brighter and more concentrated than the rest of the galaxy. The color gradient shows a yellowish-white hue towards the center, suggesting a population of older stars, while the outer regions appear slightly bluer, implying the presence of younger stars and ongoing star formation, albeit at a moderate level. The overall structure does not indicate any significant tidal disturbances or signs of recent major mergers, although there is a slight asymmetry. There is no well-defined spiral arm structure or a prominent disk.
