The galaxy presents as a centrally concentrated spheroid with a relatively smooth texture, appearing elliptical in shape. Its light profile suggests a dominant bulge component. The galaxy exhibits a reddish-yellow hue, indicative of an older stellar population and a relatively low ongoing rate of star formation. There is a slight elongation evident, moving from the bottom left to the top right. No strong spiral arm structures or significant dust lanes are visible, giving the galaxy a generally featureless appearance. There is no evidence of ongoing major mergers or significant tidal disturbances. Based on its color and morphology, it is potentially a massive, evolved galaxy, with a minimal ongoing specific star formation rate.
