The galaxy presents a disturbed morphology, exhibiting characteristics suggestive of an ongoing or recent interaction or merger. It displays a prominent, irregularly shaped disk structure, with a clear blue hue indicating active star formation regions within. These regions appear as several bright knots scattered throughout the disk, highlighting areas of intense stellar birth. Spiral arm structures are present, though somewhat disrupted and ill-defined, further supporting the interpretation of gravitational disturbance. A faint central bulge is visible. A second, more lenticular galaxy is also visible, with a much more smooth, undisturbed structure. The galaxy appears elongated and relatively featureless, presenting a yellow-orange coloration consistent with an older stellar population and little ongoing star formation.
