The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth light distribution. The core exhibits a bright, yellowish-white color, indicating a likely concentration of older stellar populations. Moving outwards from the core, the color transitions to a slightly more blueish hue, possibly suggestive of younger stars or some degree of ongoing star formation. The overall shape is somewhat elongated, appearing cigar-shaped rather than perfectly spherical, though the lack of distinct features suggests it is relatively undisturbed. There are no apparent spiral arms or prominent dust lanes visible within the galaxy's structure. The overall light profile fades gradually from the center outwards, lacking any sharp edges or abrupt truncations. The galaxy shows no visible signs of any major ongoing mergers, although subtle disturbances cannot be ruled out due to the resolution of the image.
