The galaxy presents as a smooth, elongated structure with a high degree of axial ratio. Its morphology suggests an elliptical classification, although a highly inclined disk galaxy cannot be ruled out based on this single image. The light distribution appears relatively uniform across the main body, with a subtle central concentration. The color profile shows a dominance of redder wavelengths, which may indicate an older stellar population and a relatively low rate of current star formation. There is no apparent evidence of spiral arms or significant dust lanes. No signs of ongoing major merger activity are visible, although subtle asymmetries may indicate a past minor interaction or disturbance. The galaxy's size is moderately small, suggesting a dwarf or low-mass system. 
