The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, though with a slight elongation. The light profile suggests a centrally dominant bulge. The color gradient indicates a population of older stars, with a hint of ongoing, although limited, star formation. The lack of pronounced spiral arms or significant dust lanes reinforces its classification as an early-type galaxy. There is no visual evidence of a major merger event or significant tidal disturbance. Overall, it is a relatively low-mass galaxy with a low star formation rate and an intermediate specific star formation rate.
