The galaxy presents as a slightly elongated, disk-like structure with a relatively smooth appearance. A central bulge region exhibits a more concentrated, yellowish hue, suggesting an older stellar population. Fainter, bluer light extends outward from the bulge, indicative of younger stars and potentially ongoing star formation within the galactic disk. There is a slight hint of disturbance to the symmetry of the disc, but on the whole the morphology appears undisturbed and unmerged. Based on the colors, the mass of the galaxy is somewhere in the range of 10^10 solar masses. The galaxy has a rate of star formation that is on the order of 10^1 solar masses per year.
