The galaxy appears to be a disk galaxy, viewed at a significant inclination. A central bulge is visible, exhibiting a smooth, concentrated light profile with a yellowish hue suggesting an older stellar population. Surrounding the bulge is a disk component that is bluer in color, indicating ongoing star formation. The disk appears somewhat asymmetrical, hinting at possible past interactions or internal disturbances. There are no readily discernible spiral arm structures. Overall, the galaxy exhibits a moderate level of smoothness, but displays features that suggest ongoing or recent activity.
