The galaxy presents an elongated, somewhat irregular morphology. The central region displays a brighter, more concentrated luminosity profile, suggesting a possible bulge or core structure. Distally, the galactic disk is less defined, with areas of diffuse light. There is an apparent disturbance within the disk, particularly near the upper region. The color is indicative of ongoing star formation activity, with a predominantly blue hue suggesting a population of young, massive stars. There appears to be a slight warp, possibly indicative of tidal interactions or a recent merger event with a small galaxy. The image indicates that the galaxy is likely viewed from an oblique angle, due to its elongated shape.
