The galaxy presents as a concentrated, generally smooth object with a fairly round morphology. The light distribution suggests a central bulge that transitions outwards. The colour profile indicates a mix of stellar populations. The core appears to be predominantly composed of older stars, seen by the redder light in this location. The outer regions display bluer hues, which would indicate the existence of younger stars. However, the smoothness suggests that the rate of star formation is relatively quiescent. No prominent spiral arm structures or bar features are discernible in the image, lending further support to the smooth morphology. There are no obvious signs of tidal interactions or ongoing mergers.
