The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. Its color profile suggests a relatively passive stellar population. The galaxy exhibits a slight elongation, deviating minimally from a perfect circular shape. Visual inspection suggests the galaxy does not display any prominent spiral arm structures, tidal tails, or other signs of significant ongoing or recent major mergers. There is potential evidence of minor disturbances within the galaxy's outer regions, though these are not pronounced. Overall, the morphology is indicative of a relatively evolved galaxy with limited current star formation.
