The galaxy presents a somewhat elliptical, though not perfectly round, morphology. The central bulge exhibits a bright, concentrated luminosity, appearing predominantly yellow. The outer regions display a smoother texture, with a faint red tinge discernible in one region above the bulge. There are indications of possible tidal features or minor disturbances, although the image quality limits a definite conclusion. Star formation seems to be relatively quiescent in the central region but more prominent in the region with the red tinge. A merging event appears possible. Overall, the galaxy appears to be a massive system that has a relatively old stellar population, as supported by the redder hue of the outer regions.
