The galaxy presents as a spiral type, showing a somewhat disturbed morphology. The central bulge appears moderate in size, with a noticeable deviation from perfect symmetry. Faint spiral arms are visible, exhibiting a loose structure, though these are not clearly defined or continuous. The color profile suggests a higher concentration of older stellar populations in the central regions, indicated by redder hues, with bluer regions appearing in patches along the arms, indicating recent or ongoing star formation. The disk of the galaxy is not perfectly flat; it has some minor distortions. There may be evidence of a minor merger event or tidal interaction. The overall light distribution suggests that the object is more likely to be a galaxy with notable features rather than a pure elliptical type. The overall texture of the galaxy presents a moderately smooth appearance, though subtle disturbances are present upon closer inspection.
