The galaxy presents a disk-like morphology, with a relatively bright central bulge. Faint spiral arm structures are visible emanating from the central region, with most arms exhibiting a tightly wound configuration. The disk component appears to have a slight inclination relative to our line of sight. The overall color suggests a mix of stellar populations, with a more yellow to red central bulge and a bluer disk, which is indicative of ongoing star formation. There is no visible evidence of a strong bar structure or major merging activity.
