The galaxy presents as a relatively smooth, centrally concentrated structure. The light distribution appears mostly uniform, lacking prominent spiral arms or a well-defined disk. There is a suggestion of a slight elongation, but overall, the object appears approximately round. The color gradient moves from a bright, yellowish-white core to a fainter, more reddish-hued outer region, possibly indicating an aging stellar population or dust extinction in the outskirts. The presence of low-level disturbances or features within the galaxy cannot be ruled out, but they are not readily apparent in this image. The morphological classification leans toward the smooth end of the spectrum, with a possible minor disturbance.
