The galaxy presents an overall smooth morphology, with a slightly elongated shape that is somewhere between round and cigar-shaped. The light distribution indicates a dominant bulge component, which is much brighter and concentrated than any disk. The color of the bulge is distinctly redder or yellower compared to the periphery of the galaxy, which is tinged with bluish or greenish hues. There is a suggestion of a slight disturbance of the galaxy's structure. Given the redshift, it is relatively luminous and massive. The galaxy's ongoing star formation is estimated to be low. There may be a minor merger happening.
