The galaxy presents as a centrally concentrated object, exhibiting a generally symmetrical structure with a relatively smooth appearance. There is a distinct, bright core from which light appears to emanate outwards. Faint disk-like structures can be seen at the edges of the galaxy. The galaxy's color is primarily blue-white. There is a hint of internal structure with some areas appearing slightly more disturbed. The overall morphology appears to be consistent with a spiral galaxy undergoing relatively active star formation. Evidence indicates it may be in a stage of minor interaction or merging, potentially contributing to its observed star formation rate.
