The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a concentrated, bright, yellowish hue, which fades into a diffuse halo. The overall shape is noticeably circular, indicating a lack of significant rotational features, such as spiral arms or a prominent disk. There is little visible evidence of ongoing major mergers or significant tidal disturbances. Minute, irregular features seem to emanate slightly from the central region, suggesting possible minor interactions or internal dynamic processes within the galaxy.
