The galaxy presents an irregular morphology, elongated along a single axis, and spanning approximately 4.5 kpc in diameter. The color gradient suggests a composite stellar population. The central region exhibits a yellowish-white hue indicative of older, redder stars, potentially a bulge component. Moving away from the center along the major axis, the colors shift towards blue, suggesting the presence of younger, hotter stars and ongoing star formation in these regions. Faint, diffuse extensions are visible, potentially tidal features or disrupted spiral arms, which might be indicative of a past or ongoing merger event. There are areas of minor disturbance and major disturbance, with one merging taking place. The overall structure is not well-defined, deviating significantly from a smooth elliptical or well-defined spiral structure, which is indicative of a disturbed or merging system.
