The galaxy presents as a somewhat face-on spiral structure, although its orientation is slightly inclined from our point of view. A central bulge dominates the galaxy's core, exhibiting a yellowish hue indicative of an older stellar population. The spiral arms are moderately defined, displaying hints of blueish regions which may indicate ongoing star formation within these arms. A central bar structure appears to be present, extending through the core region of the galaxy. The outer regions appear somewhat disturbed, and the appearance suggests a possible minor interaction or merging event. Overall, the galaxy exhibits a moderate degree of internal structure and features.
