The galaxy presents as a slightly elliptical, disk-like structure. A prominent central bulge is observed, exhibiting a yellowish hue, potentially indicative of an older stellar population. The outer regions of the disk appear less defined and more diffuse, showcasing a bluer coloration, suggesting ongoing star formation. There is evidence of some minor structural asymmetry or disturbance in the disk, though a clear merging event is not apparent. Overall, the galaxy appears to be relatively smooth, with some subtle features hinting at internal processes or past interactions.
