The galaxy appears to be a relatively large, elongated spiral galaxy, likely seen at an oblique angle. The central bulge is bright and somewhat diffuse, exhibiting a yellowish-white color, suggestive of an older stellar population. Fainter spiral arms extend from the bulge, with hints of bluer regions along the arms, indicating areas of more recent star formation. There seems to be some degree of asymmetry or mild distortion present, possibly due to a minor gravitational interaction. One side of the galaxy seems to have a more concentrated area with a reddish hue, possibly due to a region with a high concentration of dust or older stars. The overall morphology suggests a galaxy with an intermediate level of star formation, a prominent bulge, and arms that are reasonably well-defined, but not tightly wound.
