The galaxy appears as a centrally concentrated object with a generally smooth morphology. Its shape is somewhat elliptical, with hints of disk-like features. It has a bright central region, likely corresponding to a galactic bulge or active galactic nucleus. The color distribution indicates the presence of both older stellar populations, evidenced by reddish hues in the outer regions, and some younger, bluer stars towards the center. There is a suggestion of faint spiral arm structures or tidal tails. There is no signs of major disturbances due to merging, but there may be minor disturbances, such as smaller galaxies being pulled apart. 
