The galaxy presents a generally elongated morphology, exhibiting characteristics indicative of a disk galaxy viewed at a high inclination. The central region displays a concentrated luminosity, possibly signifying a bulge component. A dust lane is visible near the central region, bisecting the bulge, further supporting the interpretation of an inclined disk structure. Distortions are apparent in the disk, with disrupted spiral arms or tidal features extending outward from the main body. The bluer color and clumpy structures suggest sites of active star formation within the disrupted regions. The overall color index suggests a galaxy with a mix of stellar populations, including older, redder stars and younger, bluer stars. A tail of lower surface brightness material extends from the top of the galactic disk. The image suggests a galaxy that may be undergoing or have undergone a merger or interaction.
