The galaxy presents as a moderately bright, elliptical object. It exhibits a smooth, centrally concentrated light distribution, with the intensity gradually decreasing towards the outer edges. The galaxy's overall shape is elongated, appearing as a slightly flattened spheroid. There is no obvious evidence of spiral arms or a prominent disk structure. The core region appears brighter and more compact compared to the diffuse outer halo, suggesting a concentration of older stellar populations toward the center. Color gradients are subtle but noticeable, with a generally redder hue dominating the central regions and potentially hinting at older stellar populations or dust obscuration, transitioning to slightly bluer hues in the outer regions, which could signify younger stars but the trend is not prominent. There are no clear signs of ongoing major mergers or tidal disturbances, although the possibility of minor interactions or past merger events cannot be entirely ruled out based on the available image data. Overall, the galaxy morphology is consistent with that of a relatively undisturbed elliptical galaxy.
