The galaxy presents as a somewhat smooth, featureless object with a slight elongation. The color gradient suggests a concentration of older stellar populations, exhibiting reddish hues. A bluer region is present, perhaps indicating an area of recent star formation. There is a notable disturbance in the galaxy's structure. It may be the result of an ongoing or recent interaction with another galaxy. Alternatively, this may be a merger remnant. Given the relatively undisturbed shape of the main body, the interaction, if any, appears to be in its later stages.
