The galaxy presents an overall elliptical morphology with a moderately smooth appearance. The central bulge is well-defined, exhibiting a bright, concentrated luminosity. The outer regions display a gradual decrease in surface brightness, suggesting a relatively extended halo. There are hints of some substructure or irregularities within the disk, but these are subtle, not particularly prominent, and somewhat irregular. There appears to be a neighboring galaxy close to the center. The color profile suggests a slightly redder hue in the central bulge, transitioning to a marginally bluer tone toward the outer disk, which could be indicative of varying stellar populations or dust distribution. 
