The galaxy presents as a disk galaxy, viewed at an oblique angle that is not quite edge-on. There is a bright central bulge, unresolved in this image, exhibiting a high degree of luminosity. Diffuse spiral arms emanate from the bulge, extending into the surrounding disk. These arms appear somewhat flocculent, with regions of slightly enhanced star formation evidenced by a bluer hue, though the spiral structure is not sharply defined. The disk itself displays a generally smooth texture, which suggests a relatively high degree of stellar population mixing. The color of the disk is intermediate between blue and red, indicating a mix of both young and old stars and some ongoing star formation. Overall, the galaxy shows some evidence of disturbance, possibly indicating a past interaction or merger event, as the arms appear somewhat disrupted. However, a more in-depth spectral analysis is needed to confirm the rates of star formation.
