This galaxy presents as an elongated, disk-like structure. The central bulge appears luminous and exhibits a yellowish-white hue, suggesting a population of older stars. The disk component is relatively smooth in appearance with some faint spiral arm structures visible on either side of the bulge. The galaxy is tilted significantly relative to the line of sight from Earth. The galaxy is approximately 8.3 kpc in radius. Faint hints of bluer color are present at the edges of the disk indicating some ongoing star formation. There is no evidence of any major merging activity or significant tidal disturbances. Overall, this galaxy appears to be a relatively undisturbed spiral galaxy at moderate redshift.
