The galaxy exhibits a prominent spiral structure, readily identified by the presence of well-defined spiral arms. The arms appear tightly wound, originating from a central bulge. The central bulge is relatively small, with an intense, bright yellow color, likely indicating a population of older stars. The spiral arms themselves display a bluer hue, suggestive of ongoing star formation within these regions. The color gradient, transitioning from yellow to blue from center to periphery, supports the hypothesis of stellar evolution gradients within the galactic structure. There is a hint of asymmetry or disturbance in the outer regions of the disk, but no significant merger event is taking place. There is evidence of a faint bar structure crossing the central region. This galaxy appears to have a classic spiral galaxy morphology.
