The galaxy presents an elongated morphology, appearing cigar-shaped in projection. The light distribution is not uniform, with a brighter central region surrounded by a more diffuse halo. Evidence suggests a relatively smooth overall structure, although there is some indication of possible disturbances or faint features within the galaxy, indicating an ongoing or recent interaction. The color profile exhibits a gradient, with the central region showing bluer tones and the outer regions trending towards redder hues, possibly indicative of a mix of stellar populations, with younger stars concentrated towards the center. This is possibly indicative of a moderate star formation rate within the galaxy. The overall impression is of a massive galaxy experiencing some form of dynamical activity.
