This galaxy presents a somewhat elliptical morphology, appearing elongated in shape. Its light profile indicates a concentration of older stars towards the center, suggesting a prominent bulge component. The color gradient from the central bulge outwards seems to indicate ongoing, though potentially mild, star formation within the disk. Faint features suggestive of spiral arms or tidal disturbances are present, though not sharply defined. These features hint at possible past or ongoing interactions with other galaxies. Overall, the galaxy seems to be a transitional object, displaying characteristics of both spiral and elliptical galaxies. It has an estimated stellar mass of roughly 10^10 solar masses and a relatively low specific star formation rate, suggesting the galaxy is in a process of star formation quenching.
