The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a yellowish hue, potentially indicating an older stellar population. The overall shape appears round, with minimal deviation from a circular form. There are no readily apparent signs of spiral arm structures or major disturbances indicative of ongoing mergers. The galaxy exhibits a general red-sequence color, with a low star formation rate that is likely indicative of a quiescent or slowly evolving system. There is no evidence of substantial tidal features or interactions with nearby galaxies.
