The galaxy presents as a spiral galaxy, exhibiting a significant disk component and evidence of spiral arm structure. The arms appear somewhat flocculent rather than grand design, suggesting a less ordered spiral pattern. The presence of spiral arms implies ongoing or recent star formation within the disk. There appears to be moderate bulge. The disk shows a relatively blue color, indicative of a younger stellar population, while the bulge region is yellower, suggesting an older stellar population. There seems to be a lack of an apparent bar structure. There may be a minor disturbance, or the galaxy may be in the process of merging with another galaxy.