The galaxy appears as a moderately luminous object with a discernible disk structure. Its overall color is slightly blue, suggesting the presence of younger stellar populations and ongoing star formation, though perhaps at a relatively low rate. The light distribution is relatively smooth, with no distinct spiral arms or bar visible in this image, although some slight irregularities in the outer disk are present. It is elliptical to somewhat round in appearance, not highly elongated. There is no obvious major merger activity, though the slight disk irregularities may indicate a past minor interaction or disturbance. The estimated physical size indicates a relatively average galaxy, neither particularly large nor small.
