The galaxy presents as an elongated, somewhat irregular form, indicative of a disk galaxy viewed at an oblique angle. The central region appears brighter and more concentrated, exhibiting a yellowish hue which may suggest an older stellar population and potentially a higher concentration of dust. Moving outward from the center, the disk appears less defined and more diffuse. There's a subtle transition in color from the central yellow to a slightly bluer tint on the edges of the disk, possibly indicating regions of younger, hotter stars and ongoing star formation, however minimal disturbance in the morphology seems to imply that the rate of star formation is low. There appears to be a mild disturbance in the galactic form. The overall impression is of a galaxy with a substantial stellar mass.
