The galaxy presents as a generally smooth object with a hint of ellipticity. There is a slight deviation from perfect circularity, tending toward a slightly elongated form. No distinct spiral arms or bar structures are discernible in the image. The light distribution appears relatively even across the main body of the galaxy, with no significantly brighter central bulge. The lack of strong features may indicate a relatively quiescent galaxy, possibly with a low star formation rate. There are some indications of minor disturbances in the galaxy's morphology, but it is likely not currently undergoing a major merger event. The color suggests an evolved stellar population.
