The galaxy presents as a spiral type, observed at an oblique angle. A prominent central bulge is visible, exhibiting a yellowish hue, indicative of an older stellar population. The disk is characterized by distinct spiral arms. These arms appear asymmetric, with some showing signs of flocculence and varying degrees of definition. Patches of blue are observed within the spiral arms, suggestive of active star formation regions. Evidence of a bar structure is present, bisecting the central bulge. Overall the galaxy exhibits a moderate level of star formation, and is undisturbed.