The galaxy presents as a relatively compact and moderately luminous system. Its overall morphology appears to be primarily smooth. There is a slight, almost imperceptible elongation, suggesting it is not perfectly spherical. The light distribution within the galaxy is fairly uniform, with a gradual falloff from the central regions towards the periphery. There are no prominent spiral arms or distinct features immediately obvious in this image, and it is possible that the system exhibits some signs of minor tidal disturbances or interactions with other galaxies, based on some asymmetric light. This galaxy is likely a massive system with an active star formation rate.
