The galaxy presents a disk-like morphology with a discernible bulge. There is evidence of spiral arm structure. It seems that it may be undergoing some minor disturbance, possibly from a recent interaction. The colors indicate a mix of stellar populations, with a prominent central region that appears yellower, suggestive of older stars. The outer regions of the disk show bluish tones, potentially indicating ongoing star formation. There is evidence of some dust lanes. The galaxy is observed at an angle, suggesting it is not quite edge-on. There is a relatively smooth appearance.
