The galaxy presents a notable central bulge, exhibiting a bright, concentrated luminosity. Extending outwards from the bulge, a somewhat less defined disk is visible, displaying hints of spiral structure although its morphology appears disturbed or irregular. Color gradients are observed, with the central bulge presenting a yellowish or reddish hue, indicative of an older stellar population. The outer disk regions show bluer tones suggesting younger stars and possible ongoing star formation. The galaxy appears to be undergoing some form of interaction or disturbance that may be associated with the complex shape.
