The galaxy presents as a spiral type, exhibiting a central bulge that appears yellowish in color, suggestive of an older stellar population. Extending from the bulge are prominent spiral arms, defined by a bluer hue which indicates regions of active star formation. The arms are relatively well-defined and tightly wound closer to the bulge, becoming less defined toward the outer regions of the galaxy. There is some asymmetry in the arm structure suggesting possible interactions or internal dynamics affecting its shape. Dust lanes are not clearly visible, which could be due to the viewing angle or overall dust content of the galaxy. Overall, the galaxy appears as a relatively normal spiral galaxy with ongoing star formation within its spiral arms.
