The galaxy presents an elongated morphology, with a noticeable central bulge of concentrated light. A fainter, diffuse halo surrounds the central region, appearing more extended along the major axis of the galaxy. The color distribution suggests a gradient, with the central bulge exhibiting a yellowish hue, indicative of an older stellar population. Along the galactic disk, there are hints of bluer regions that are indicative of younger stars. There may be a slight disturbance present in the outer disk, and it is unclear whether this galaxy is a result of an ongoing merger. The galaxy does not show a well-defined spiral arm structure in this image, possibly due to the viewing angle and depth of the image.
