The galaxy presents a largely smooth, elliptical morphology. It appears relatively undisturbed, with no obvious signs of ongoing major mergers or significant tidal disruptions. The galaxy exhibits a dominant spheroidal component, suggesting an older stellar population. There is a lack of prominent spiral arm structures or distinct dust lanes. A minor blue component may indicate some ongoing, though suppressed, star formation. The galaxy's color is generally redder, hinting at a dominance of older, redder stars. Overall, this galaxy seems to be a relatively quiescent system.
