The galaxy appears as a slightly elongated, disk-like structure. The central region exhibits a concentrated, bright luminosity, suggesting a prominent galactic nucleus or bulge. The overall color profile indicates a mix of stellar populations. The central bulge has a yellowish-white hue, indicative of older stars. Surrounding the nucleus, a bluer disk component is visible, potentially containing younger stars and regions of ongoing star formation. The outer edges of the disk appear relatively smooth, lacking significant spiral arm structures. The overall shape suggests an intermediate type between a pure elliptical and a spiral galaxy, possibly an S0 or early-type spiral. The low level of visible disturbances suggests that the galaxy is relatively settled, without recent major merger events.
