The galaxy presents as a predominantly smooth, elliptical structure with a bright, concentrated core. It exhibits a yellowish-orange hue, potentially indicating an older stellar population. The overall shape appears somewhat elongated. There is a subtle hint of possible disturbances in the outer regions, though not overtly pronounced, such as tidal tails or merging signatures, as indicated by the data. No clear spiral arm structures are discernible. The mass appears substantial. Star formation rate is estimated to be quite low.
