The galaxy presents as a centrally concentrated, elliptical morphology. The light profile appears relatively smooth, with a high degree of central concentration, transitioning gradually to fainter outer regions. The overall shape is elongated, resembling a cigar-like appearance. There is no obvious evidence of spiral arm structure or significant dust lanes. A subtle color gradient is observed, shifting from a more yellowish hue in the core to a slightly bluer tint in the outer regions. There is no indication of strong tidal features or ongoing major merger activity; however, the possibility of minor disturbances cannot be ruled out. The observed characteristics are consistent with a massive galaxy exhibiting low star formation activity.
