The galaxy appears as a relatively smooth and rounded object. There is a concentration of light towards the center, which fades gradually towards the edges. The color profile seems to be dominated by yellow and red hues, suggesting a population of older stars and potentially a lower rate of ongoing star formation. No distinct spiral arms or bar structures are clearly visible. There may be a slight deviation from perfect circularity, but overall the galaxy presents a largely undisturbed morphology. Possible signs of a very minor disturbance.
