The galaxy presents a relatively smooth and centrally concentrated morphology. The overall shape appears to be somewhere between round and elliptical, with a slight deviation from perfect circularity. There's a clear central bulge region exhibiting a bright, relatively uniform emission. Surrounding the bulge, we observe a ring-like structure that is notable for its distinct color variations. The outer edges of the ring appear redder, contrasting with the bluer emission closer to the central region. There's no indication of any major merger activity or significant tidal disturbances that could be visibly deforming the galaxy's structure. The galaxy likely possesses a moderate stellar mass and a relatively low star-formation rate. The structure is likely composed of a relatively old stellar population, with younger stars concentrated in the ring.
