The observed galaxy presents as a spiral type, viewed at an oblique angle relative to its disk.  Spiral arms are discernible, exhibiting a somewhat flocculent structure.  The central bulge region appears prominent and exhibits a yellowish color, suggesting an older stellar population. The spiral arms display bluer hues, indicative of ongoing star formation.  The disk appears relatively undisturbed, though some irregular features may be present.  There is no strong visual evidence of a central bar structure. The overall morphology suggests a galaxy undergoing active star formation within its spiral arms.
