The galaxy exhibits a generally smooth morphology, with no distinct spiral arms or bar structures readily apparent. It appears largely elliptical in shape, presenting a high degree of circularity. A radial color gradient is visible, transitioning from a concentrated yellowish-white core outwards to more subdued reddish hues in the outer regions. The light profile suggests a relatively evolved stellar population. There is no strong evidence of ongoing major mergers or significant tidal disturbances. The galaxy appears relatively isolated, suggesting a lower likelihood of recent or ongoing interactions influencing its morphology. Based on its color and overall structure, this galaxy is consistent with being a relatively massive elliptical galaxy with suppressed star formation activity.
