The galaxy exhibits a disturbed morphology, possibly indicative of an ongoing or recent interaction or merger event. There is a primary, elongated component with a relatively smooth light distribution, though with some irregularities suggesting it is not a perfect ellipse. A secondary, more compact component is also visible, characterized by clumpy and irregular features, with a distinct color profile suggesting active star formation regions. Overall, the galaxy demonstrates asymmetric features in its light distribution, likely arising from tidal distortions. There is an indication of a dust lane or obscured region in the main galaxy. The color gradients suggest a population of older stars in the central regions and younger, bluer stars in the distorted or interacting regions.
