The galaxy appears as a disk-shaped structure, oriented approximately edge-on relative to our line of sight. There is evidence of a central bulge, which seems to be of moderate size. The disk exhibits a complex structure with subtle color variations, indicative of varying stellar populations. The inner regions seem to be bluer and more active, which may indicate the presence of younger stars and ongoing star formation, while the outer disk presents a more subdued color, probably from older stars. There appears to be no significant sign of tidal disturbances.
