This appears to be a spiral galaxy, exhibiting a well-defined disk structure. The spiral arms are prominent and tightly wound around a bright central bulge. The bulge appears to be of moderate size compared to the overall disk. Dust lanes are visible within the spiral arms, contributing to their complex structure. The overall color suggests the presence of both older stellar populations in the bulge and younger, bluer stars within the spiral arms, indicative of ongoing star formation. The disk is not precisely face-on, but rather oriented at a slight angle relative to the observer, though not highly edge-on. There does not appear to be evidence of a strong bar structure within the central region. There are some hints of disturbances in the outer arms suggesting a possible past merger event.
