The galaxy presents as a somewhat elliptical, smooth object with a slightly elongated morphology. The core exhibits a bright, concentrated luminosity, suggestive of a significant central mass concentration. There is a faint hint of blue hue, especially in the central region, which could indicate the presence of younger stars and ongoing star formation. The outer regions appear more diffuse, with a gradual decline in surface brightness toward the edges. The overall structure suggests a system that is neither a pure elliptical nor a well-defined spiral, but rather something in between, possibly a lenticular galaxy with characteristics of both or an elliptical galaxy in the process of formation. Possible signs of minor tidal disturbances can be observed in its overall morphology.
