This galaxy exhibits a generally smooth morphology, with a centrally concentrated light distribution. The shape approximates round, though a slight elongation is apparent, trending towards an intermediate elliptical form. No distinct spiral arms or bar structures are readily discernible. The galaxy displays a color gradient, appearing bluer in the outer regions and redder towards the center, which may indicate differential stellar populations and ongoing star formation in the galaxy's periphery. There is no compelling visual evidence for ongoing major merger activity, though a subtle asymmetry and possible minor disturbance cannot be entirely ruled out. The overall structure suggests a galaxy that has largely settled into a stable configuration.
