The galaxy presents as a face-on spiral with a redshift of approximately 0.108. Spiral arms are clearly visible, and it is likely there are three prominent arms. These arms exhibit a generally tight winding pattern. A central bulge appears prominent, occupying a moderate portion of the overall galactic disk. The nucleus is bright, suggesting the presence of an active galactic nucleus or a high concentration of stars. The disk itself shows a bluer hue, indicative of ongoing star formation. The galaxy disk is not perfectly smooth, and shows that there are some minor disturbances, but there are no signs of major mergers or significant tidal disruptions. The image reveals a generally well-defined spiral structure, with a classification leaning towards a classic spiral morphology.
