The galaxy presents as a central, moderately luminous object with a diffuse appearance. Its shape is neither distinctly elliptical nor spiral, leaning towards a more amorphous or irregular morphology. The light distribution suggests a relatively smooth profile with a slight central concentration, although some subtle features may be present. There is a faint, blueish hue associated with it, which suggests the presence of relatively young, hot stars and ongoing star formation. It is likely a galaxy that has experienced some sort of disturbance or interaction, evidenced by the asymmetry and subtle features. It exhibits no strong signs of a major ongoing merger, but the possibility of a minor interaction or past merger cannot be excluded.
