The galaxy presents as a somewhat smooth, centrally concentrated object, with a hint of a slightly elongated, elliptical shape.  It appears to be generally featureless, showing no distinct spiral arm structures or prominent dust lanes.  There is a subtle color gradient noticeable, with the central region appearing marginally more yellow-reddish compared to the slightly bluer, fainter outer regions. The galaxy is relatively isolated, showing no signs of recent or ongoing major mergers, although minor disturbances can not be ruled out. Overall, the observed characteristics suggest that this is likely a relatively massive galaxy with a fairly moderate rate of star formation.
