The galaxy appears to be a spiral galaxy, viewed at a slight angle to face-on. A central bulge is visible, exhibiting a yellowish hue, indicative of an older stellar population. The spiral arms are not tightly wound, appearing somewhat flocculent and less distinctly defined. There is evidence of on-going star formation within the arms, indicated by the presence of bluer regions, which may indicate younger, hotter stars. The galaxy displays a moderate level of internal structure with no obvious signs of a major merger event, although subtle disturbances may be present. The overall color gradient shifts from yellow in the bulge to bluer in the outer arms. It is likely a massive galaxy, with moderate star-forming regions distributed throughout the spiral arms.
