The galaxy presents an elliptical morphology, appearing largely smooth and rounded in shape. A concentrated central bulge is visible, exhibiting a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy appear fainter and less defined, with a subtle disk structure that exhibits a blueish hue. The galaxy does not appear to display any prominent spiral arms or significant dust lanes. There is no evidence of any major ongoing merger activity, although some minor disturbances cannot be ruled out based on the image quality. Overall, the galaxy presents a relatively undisturbed and evolved structure.
