The galaxy presents a largely smooth and rounded morphology. There appears to be a distinct central bulge, characterized by a brighter, more concentrated light profile. The overall color of the galaxy tends towards the redder end of the spectrum. No clear spiral arm structure or significant dust lanes are discernible in the image. There appears to be a subtle extension of light surrounding the central bulge, suggesting the presence of a faint halo. The galaxy's symmetrical appearance suggests a relaxed system, lacking obvious signs of recent major mergers or significant tidal disturbances. There is potentially a slight amount of disk character. 
