The galaxy presents as a spiral, exhibiting a clearly defined disk structure. The central bulge appears moderately prominent and is primarily a yellow-white hue, suggesting an older stellar population dominating the core. Spiral arms extend outward, primarily a blue-white color, implying active star formation. The arms are somewhat tightly wound and can be traced. There are indications of at least two arms present, possibly three. The galaxy displays an overall elliptical shape, indicating a tilt relative to our line of sight. It is not perfectly edge-on, nor face-on. There are no obvious signs of tidal disturbances or major mergers. The galaxy exhibits no apparent bar feature bisecting the central bulge. Dust lanes or patches may be present within the spiral arms, but image resolution limits definitive identification.
