The observed galaxy presents a defined but diffuse spiral structure. While not perfectly face-on, the disk is presented with some tilt. There is evidence of prominent spiral arms extending from the central bulge, appearing somewhat flocculent and not sharply defined.

The central bulge is relatively bright and appears yellow in color, suggesting an older stellar population. The disk shows a bluer hue overall, indicating ongoing star formation regions along the spiral arms, although this is not strongly pronounced. The spiral arms exhibit some patchiness. There appears to be no strong evidence of a central bar structure, although weak features may be present. There also appears to be a moderate bulge.

There are irregularities in the overall shape of the galaxy, suggesting possible minor gravitational interactions or disturbances. These distortions are not major, but indicate a system that may have experienced a recent merger. The overall morphology suggests a system that is neither a pure elliptical galaxy nor a pristine spiral, showing intermediate characteristics.
