The galaxy presents as an elliptical structure with a relatively smooth, featureless appearance. There is an indication of an oblate spheroidal shape; the galaxy is more 'in-between' round and cigar-shaped. The color gradient suggests a slightly redder hue towards the center of the galaxy, potentially indicating an older stellar population concentrated within the core. The disk features are not clearly distinguishable in this image. It does not appear to be undergoing a major merging event, though minor disturbances cannot be ruled out. The galaxy's light profile suggests a moderate level of star formation activity.
