The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light profile appears to decrease gradually from the core outwards. The primary color is a yellow-orange hue suggesting an older stellar population. There is a subtle indication of a slight disk-like structure. No prominent spiral arms are evident. No signs of ongoing major mergers or significant tidal disturbances are apparent. The galaxy appears to be in a relatively quiescent state. 
