The galaxy appears to be in the process of merging or undergoing a significant interaction. Morphologically, it presents with disturbed features, potentially indicating tidal effects. The shape is somewhat elongated, trending towards a cigar shape rather than a perfect circular or elliptical form. It possesses an apparent smooth component, but also exhibits features indicative of disk or spiral structure. The color profile suggests ongoing star formation. Given the inferred size and luminosity, the galaxy likely possesses a significant stellar mass. A slight color gradient is visible, suggesting variations in stellar population or dust content across the galaxy.