This galaxy presents as a spiral galaxy. The central bulge appears moderately prominent, with a yellow-white hue, suggesting a population of older stars. Two well-defined spiral arms emanate from the central bulge, tracing a relatively open, medium-winding pattern. The arms are tinged with bluer light, indicating regions of active star formation. There is evidence of a bar-like structure extending from the center of the galaxy, adding to the complexity of its morphology. Overall, the galaxy exhibits a classic spiral structure with ongoing star formation within its arms. There are no obvious signs of major disturbance or merging events. The light distribution suggests a smooth transition in stellar population density, with the bulge containing a higher concentration of older stars and the arms highlighting regions of active star formation.
