This galaxy appears to be a spiral galaxy viewed at an angle that is oblique, but not quite edge-on. The disk component is clearly visible, exhibiting distinct spiral arm structure. The spiral arms are fairly tightly wound, and it is difficult to discern their exact number. The galaxy is likely composed of two major arms. The central bulge appears somewhat moderate in size and has a slight yellowish hue, which implies the presence of an older stellar population, which indicates star formation has been occurring for a long time. The disk shows bluer regions interspersed between the spiral arms, suggesting ongoing star formation activity in those areas. Overall, the galaxy appears relatively undisturbed, though there are some asymmetries to the spiral arm structure. The color distribution suggests a range of stellar populations within the galaxy, from older stars in the bulge to younger, bluer stars within the spiral arms. There may be a bar-like feature present, although it is not prominently defined. The overall shape is elongated, consistent with a spiral disk viewed at an oblique angle.
