The galaxy presents as a somewhat flattened, disk-like structure oriented at an oblique angle to our line of sight. The central bulge appears relatively small and indistinct. The color profile of the galaxy suggests a potential variation in stellar populations. The central region exhibits a bluer hue, possibly indicative of younger, hotter stars and ongoing star formation. Moving outward from the center, the colors shift towards redder tones, possibly indicating older stellar populations. The galaxy may be interacting with a small irregular galaxy or perhaps a large globular cluster. The presence of this secondary object suggests a possibility of tidal interactions affecting the overall morphology of the larger galaxy. There is a clear disturbance in the halo of the primary galaxy near the suspected interacting galaxy. The overall smoothness suggests that it has already passed a "smoothness" threshold.
