The galaxy exhibits a generally smooth morphology, yet it appears to show some disturbances to its structure. The galaxy's shape is somewhat elongated. The central region has a relatively high concentration of luminosity, suggesting a bulge. There are some regions appearing to be dusty, which is likely the cause for the irregular structure. Some areas present a bluer hue which may correspond to areas of higher star formation. Overall, the galaxy presents characteristics indicating a history of some form of disruption or interaction.
