The galaxy presents as a fairly smooth, elliptical-like structure, exhibiting a concentrated central bulge that graduates outward into a less defined halo. The primary color gradient transitions from a yellow-white core to a redder outer region. There is some evidence of slight elongation. No distinct spiral arms or significant dust lanes are discernible within the given image resolution, nor is there evidence of tidal disturbance or close interaction with other galaxies. It displays an overall high degree of central concentration.
