The observed galaxy exhibits an irregular morphology. A central, bright core is clearly visible, emitting strongly in the blue wavelength, surrounded by a less luminous halo, extending approximately 2.7 arcseconds in diameter. This halo presents some structure, with filamentary features extending outwards. The overall color is predominantly blue-green, suggesting active star formation within the galaxy. There is also an indication of a possible tidal tail or disturbance on one side of the galaxy, marked by a slight color shift towards the red wavelength. The features are not distinctively smooth, but more of a disturbed structure indicating a possible ongoing minor merger event. The galaxy's shape suggests a distorted disk structure with a bright central bulge, though a definitive classification is difficult given its disrupted appearance.
