The galaxy presents as a relatively small, faint object with an estimated effective radius of approximately 9 arcseconds. Its overall morphology appears to be disk-like, although its detailed structure is poorly resolved in the image. The galaxy exhibits a mixed color profile, with a slightly bluer central region transitioning to redder colors in the outer areas. There is a slight suggestion of disturbance within the disk, potentially indicative of minor interactions or internal asymmetries. This disturbance appears as a non-uniform brightness distribution rather than distinct tidal features. Overall, the image suggests a galaxy that is either relatively distant, faint, or undergoing some kind of dynamic process.
