The galaxy presents a disk-like morphology, viewed at a significant inclination. A central bulge is evident, exhibiting a yellowish hue, potentially indicative of an older stellar population. The disk component displays a bluer color, suggesting the presence of ongoing star formation. A dark lane is visible on one side of the galaxy, likely due to dust obscuration within the galactic plane. The overall structure appears relatively smooth with faint spiral arms. The galaxy seems to be generally undisturbed with no major signs of merger activity.
