The galaxy presents a morphology characterized primarily by a smooth, elliptical-like structure. A central, concentrated bulge region exhibits a bright, yellowish-white hue, suggesting a population of older stars. The overall shape of the galaxy leans towards being in between round and elliptical. There is faint structure indicating that a disk may be present, but this is minimal. A possible disturbance appears on one side of the disk, but otherwise it appears to be stable. Its color indicates active star formation in areas outside of the bulge. Overall, the object gives the impression of being a relatively evolved system, but still actively forming stars.
