The galaxy presents as a generally smooth object, elongated in shape with an approximate axis ratio of 0.6. A central bulge is discernible, appearing yellowish-white and brighter than the rest of the galactic disk. The disk itself exhibits a bluer hue on the edges furthest from the center, possibly indicating regions of recent star formation. The galaxy does not display any obvious spiral arm structures or strong dust lanes, and it shows no major morphological disturbances, suggesting that it may be undisturbed and is not currently undergoing a major merging event. Overall, the galaxy is likely a relatively massive system with a moderate rate of star formation.
