The galaxy presents a somewhat amorphous morphology, lacking a distinct spiral arm structure or a prominent central bulge. The light distribution appears relatively smooth with some clumpy regions, indicating possible areas of higher star formation activity. It displays a general flattened shape. The galaxy appears to be in a relatively quiescent state, showing a low star formation rate. Based on the light profile, the system has an estimated stellar mass around 10^9 solar masses. There is a suggestion of some minor disturbance or interaction, though a major merger event is less likely based on its morphology. The colours observed suggest a mixture of stellar populations, with relatively more contribution from older stars.
