The observed galaxy presents an elongated morphology, suggesting a possible disk-like structure viewed at an oblique angle. There is a notable color gradient, with the central region exhibiting a yellowish hue that gradually transitions to a bluer tint towards one end of the galaxy. This color variation could be indicative of differential stellar populations, with older, redder stars concentrated in the core and younger, bluer stars residing in the outer regions, potentially within spiral arms. The galaxy appears relatively smooth in overall texture, although there is a suggestion of some irregular structure. Possible merger activity cannot be ruled out given these factors.
