The galaxy presents a generally smooth, elliptical morphology, exhibiting a concentrated central bulge that appears yellowish-white. Fainter, bluer emissions suggest the presence of some star formation activity within the galaxy, though it is not the dominant feature. There is evidence of a disk, but it is difficult to discern more structural details. Minor asymmetrical light patterns suggest there might be a recent minor disturbance. There is no significant visual indication of spiral arms or a major merger event currently in progress.
