The galaxy presents as a relatively compact and luminous object. Its morphology appears predominantly smooth, with a high degree of circularity. There is a subtle color gradient, trending towards a slightly redder hue in the central region, indicating a potential concentration of older stellar populations. No distinct spiral arms or bar structures are discernible within the resolution of the image, suggesting either an elliptical or lenticular classification. There is no clear evidence of ongoing major mergers or significant tidal disturbances in the image. The overall impression is that of a well-evolved, quiescent galaxy.
