The galaxy presents a prominent, bright central bulge, exhibiting a yellowish hue suggestive of an older stellar population. Extending from this central region are two well-defined spiral arms. The arms are tightly wound and have a medium pitch angle. The overall structure indicates a generally undisturbed disk morphology. The spiral arms display variations in color, interspersed with regions of bluer emission indicative of recent star formation. The galaxy is moderately inclined relative to our line of sight, allowing a clear view of its spiral structure. There is no discernible major merger or disturbance within the system, with only minor asymmetries noted in the outermost regions. The overall color profile suggests a system actively forming stars, but with a considerable population of older stars residing primarily in the central bulge. A weak bar structure appears to be present.
