The galaxy presents a generally smooth and elliptical morphology. It exhibits a bright, concentrated central bulge, indicative of a significant stellar population. There's a gradual decrease in luminosity from the core outwards, lacking any prominent spiral arm structure or distinct features associated with active star formation in the disk. The galaxy appears quite round, with only slight deviation from a perfect circle. There's no strong evidence of any major ongoing merging activity, though subtle disturbances could be present in the outer regions. The overall color profile seems relatively red, suggesting an older stellar population with minimal recent star formation.
