The galaxy presents a smooth, elliptical morphology. It appears to be a relatively concentrated object, with a bright, well-defined core region and a noticeable decrease in surface brightness moving outwards towards its periphery. There is a slight elongation to the galaxy's shape, indicating it is not perfectly spherical. The light profile suggests a bulge-dominated system. The color gradient appears to be relatively uniform, with a subtle shift towards redder hues in the outer regions as opposed to the inner regions that show slightly bluer hues. There is no evidence of spiral arm structure or prominent dust lanes. The overall structure points to a relatively evolved galaxy, consistent with a lack of significant ongoing star formation. The galaxy’s structure is largely undisturbed, with no apparent signs of recent or ongoing major mergers, although there may be some minor distortion on one side.