The galaxy presents as a spiral, viewed at an inclined angle relative to our line of sight. A central bulge is visible, appearing moderately prominent and exhibiting a yellowish hue, indicative of an older stellar population.

Spiral arms emanate from the central bulge, showing a tightly wound morphology. These arms are distinguished by their bluer color, suggesting ongoing star formation activity within these regions. The arm structure appears somewhat flocculent, with sections that are not well-defined and exhibit interruptions.

There are areas of active star formation, seen as subtle variations in color and brightness along the spiral arms. The overall appearance suggests a galaxy of significant mass, and the well-defined bulge indicates an advanced stage in its morphological evolution, despite signs of continued star formation within its spiral arms.
