The galaxy presents as a somewhat elliptical, concentrated structure. Its core exhibits a bright, yellowish-orange hue, indicating a potentially older stellar population dominating the central region. The galaxy's outer regions display a less defined boundary, fading into the background sky. Fainter, more diffuse structures are hinted at in the outer regions, possibly representing extended stellar halos or tidal features resulting from past interactions. There is minimal evidence of spiral arm structure. The overall color suggests a relatively low rate of current star formation. The system does not appear to be undergoing a major merger event; there is low incidence of dramatic disruptions to its overall shape.
