The galaxy presents as a relatively compact structure. It appears to possess a subtle disk-like morphology, though without prominent spiral arm features visible in this image. The galaxy exhibits a moderate degree of central concentration, with the luminosity appearing to be brightest in the central region. There may be a small amount of disrupted or irregular material present, but this feature is not extremely pronounced. Its ellipticity is relatively low, meaning it is more circular than elongated. Overall, it looks to be a typical galaxy at a great distance.
