The galaxy presents an elongated, cigar-shaped morphology. It appears largely smooth in texture, displaying a concentrated central bulge that emits strongly. The light appears to be reddened, implying the presence of older stellar populations. There may be hints of a disk-like structure, although it lacks prominent spiral arms or distinct features. Weak star formation is a possibility, but without more information, this is unclear. Overall, the galaxy appears relatively undisturbed, with no strong signs of recent or ongoing mergers.
