This galaxy exhibits a lenticular morphology, displaying a prominent central bulge surrounded by a flattened disk. The bulge component appears luminous, with a concentrated, yellowish-white hue, suggesting a population of older stars. The disk, observed at an oblique angle, shows a faint, diffuse spiral structure. The overall color distribution indicates a moderate amount of ongoing star formation, although the lack of intense blue regions suggests that star formation is not the dominant process within the galaxy. The galaxy appears relatively isolated, lacking any obvious signs of interaction or tidal disturbances.
