The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. It exhibits a noticeable color gradient, transitioning from a bright, yellow-orange core to a dimmer, slightly reddish outer halo. There is minimal evidence of spiral arm structures or significant dust lanes visible in this image. The galaxy appears to be quite rounded in overall shape, exhibiting a high degree of symmetry. There are no readily apparent signs of ongoing major merging events or strong tidal disturbances. The galaxy displays characteristics consistent with an evolved system, potentially with a suppressed star formation rate.
