The galaxy presents as a spiral, seen at a significant angle of inclination relative to our line of sight. The central bulge appears bright and concentrated, exhibiting a yellowish-white hue suggestive of an older stellar population. Fainter spiral arms extend outwards from the bulge. These arms are subtly bluer in color, potentially indicative of ongoing star formation. There's a general smoothness to the overall morphology, though some slight asymmetry is visible in the arm structure, possibly the result of a minor interaction. The disk is thin and extends for a moderate distance relative to the size of the central bulge. No prominent dust lanes are easily discernible. The overall structure indicates a galaxy that is neither fully quiescent nor undergoing intense starburst activity, but instead demonstrates a moderate level of star formation within its spiral arms.
