The galaxy presents as a disk galaxy, viewed at an oblique angle. The central bulge appears moderately prominent and exhibits a yellowish hue, suggesting an older stellar population. Surrounding the bulge, the galactic disk displays a distinct spiral structure, evidenced by bluer regions indicating the presence of younger, hotter stars within the spiral arms. Some arms appear flocculent, with a somewhat disorganized structure. The galaxy is relatively bright and appears to be surrounded by a diffuse halo or envelope of light. There is no apparent evidence of ongoing major merging activity, though subtle asymmetries might suggest minor tidal interactions. The overall morphology points towards a galaxy that is largely undisturbed, exhibiting relatively well-defined spiral arms and a settled structure.
