The object presents as a spiral galaxy with a substantial disk component and a noticeable central bulge. The galaxy is observed at an inclination angle, offering a somewhat oblique view of the disk structure.

Within the disk, spiral arms are discernible, exhibiting a relatively open winding pattern. These arms appear somewhat flocculent and asymmetric, exhibiting varying degrees of definition and branching. There is an indication of ongoing star formation activity within the spiral arms, evidenced by localized regions of bluer light.

The central bulge appears to be a moderate fraction of the galaxy. The color suggests an older stellar population. The surface brightness gradually increases toward the center, culminating in a bright nucleus.

Overall, the galaxy appears relatively undisturbed. While there is some asymmetry in the spiral arm structure, there are no obvious signs of major interactions or mergers affecting its morphology.
