This galaxy exhibits a spiral morphology, presenting a clear disk structure. Prominent spiral arms are visible, though somewhat tightly wound. There appears to be a notable bulge component, moderate in size, contributing significantly to the overall luminosity. The galaxy's color suggests a mix of stellar populations, with a central, yellower region indicative of older stars and a bluer hue in the outer spiral arms, potentially indicating ongoing star formation. No strong bar feature is immediately apparent. Some minor disturbances may be affecting the system.
