The galaxy appears as a centrally concentrated object with a smooth morphology. The central region exhibits high surface brightness, potentially indicative of an active galactic nucleus or a dense stellar population. There is evidence of a faint, extended halo surrounding the core, with a slight elongation along one axis. In color, the core is a blue-white, while the outer regions of the halo display more green and blue. There appears to be some irregularities in the outer regions, possibly hinting at minor disturbances. The disk is nearly face on from our viewpoint.
