This galaxy exhibits a disk-like morphology, appearing somewhat lenticular. The central region presents a bright, concentrated bulge, indicating a high density of stars. The disk appears relatively smooth. There are no prominent spiral arm structures visible. Some faint, blue-tinged regions are located along the periphery of the disk, possibly indicating areas of more recent star formation. There seems to be no significant evidence of ongoing major merger activity, although minor disturbances can not be ruled out.
