The galaxy presents as a face-on spiral with a prominent, moderately sized bulge exhibiting a yellow hue, likely indicating an older stellar population within. Two distinct spiral arms emanate from the central bulge, displaying a somewhat loose winding pattern. These arms are populated with regions of blue, suggesting the presence of ongoing star formation. There appears to be no strong central bar feature. The overall disk of the galaxy shows evidence of some disturbance, potentially indicating a minor interaction or merger event in its past. The galaxy displays a clear disk morphology, not a spheroidal shape.
