The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a roughly elliptical morphology, with a bright, compact core region that likely corresponds to the galactic nucleus. There may be a subtle hint of spiral structure or an extended disk component. The overall color suggests a moderate level of star formation activity, though the precise age distribution of the stellar populations cannot be determined from the available image resolution. A slight irregularity on one side of the galaxy could indicate a minor interaction or disturbance, but this feature is not distinctly defined. The galaxy is likely a moderate-mass system.
