The galaxy presents as a spiral galaxy, viewed at a considerable inclination. A moderately sized bulge is apparent at the center, exhibiting a yellowish-orange hue indicative of an older stellar population. Faint spiral arms extend outward from the bulge, displaying a bluer color, which suggest younger, hotter stars and star-forming regions. The arms are somewhat indistinct and appear less tightly wound, possibly indicating a grand-design or flocculent spiral structure. There is no obvious sign of a strong bar feature. The overall appearance is relatively smooth, with only minor disturbances or distortions visible, suggesting the absence of any major recent merger activity. The galaxy presents a defined central region, suggesting there has been a period of quiescence.
