The galaxy presents as a spiral type, with a distinct, though somewhat obscured, disk structure. The disk exhibits a bluish hue, suggestive of ongoing star formation activity. Two prominent spiral arms are visible, exhibiting a medium winding pattern. The central bulge appears prominent, displaying a yellowish-white color, indicative of an older stellar population. There is evidence of a bar-like structure crossing the central bulge, with a moderate strength. No signs of major merging events are discernible, though subtle irregularities within the disk might indicate minor disturbances or past interactions. Overall, the morphology suggests a relatively undisturbed spiral galaxy, with a moderate bulge and active star formation within its spiral arms.
