The galaxy presents as a spiral with a significant disk component. The disk appears inclined relative to our line of sight, exhibiting an elliptical shape. Spiral arms are present, though somewhat loosely defined and flocculent in nature. There may be weak bar structure towards the galactic center. The central bulge is moderate in size and has a smooth texture. The color gradient suggests a population of older stars and lower rates of star formation. There are no obvious signs of major mergers or tidal disturbances in the overall morphology. The galaxy appears relatively isolated in the image, with no clear interacting companions.
