The galaxy exhibits a generally smooth morphology, with some indications of features possibly attributable to a disk or disturbances. It presents a moderately elongated shape, somewhere between round and cigar-shaped, but not perfectly circular. The primary structure shows a central region with a bright, concentrated luminosity, and the overall light distribution is relatively uniform, lending to the classification of being "smooth". However, there is some unevenness to the luminosity, suggesting possible structural features. There are also a couple of offshoots or disturbances to the right of the galaxy. There is no clear evidence of ongoing major merging activity, but the possibility of minor disturbances cannot be excluded. The color indices show a generally redder overall color, and with the redder color, one part of the galaxy (to the right) could also be classified as having the color of a disturbed galaxy.
