The galaxy appears to be a spiral galaxy, viewed at an oblique angle.  A distinct bulge is not obvious, but there is some central concentration of light.  The arms are not well-defined, appearing somewhat flocculent.  One side of the galaxy is more luminous and bluer in color compared to the other side, which displays a yellower hue, possibly indicating differential star formation rates or dust obscuration. There is no obvious sign of a recent major merger, but perhaps a possible minor disturbance. The overall shape could be described as somewhat rounded or lenticular, with slight elongation.
