The galaxy presents as a relatively smooth, elliptical structure. The central region displays a high surface brightness, suggesting a dense concentration of stars. Moving outward from the core, the brightness gradually decreases, indicating a radial falloff in stellar density. There's a slight elongation to the galaxy's shape; it is somewhere in between round and cigar shaped. The color appears to be largely homogenous, with only subtle variations. The lack of prominent blue regions suggests a relatively low ongoing star formation rate. There is no sign of tidal features or merging events. Overall, the galaxy exhibits characteristics consistent with a mature elliptical galaxy.