The galaxy presents as a centrally concentrated, relatively smooth object. It exhibits a slightly elliptical morphology, appearing nearly round but with a subtle elongation. The core region displays a bright, blue-ish color, suggesting the presence of a population of young, hot stars or a possible active galactic nucleus. Surrounding the central region, the galaxy displays a gradual decrease in surface brightness, transitioning to a fainter halo or outer disk. There is faint structure surrounding the central core, but it appears largely featureless without prominent spiral arms or distinct morphological disturbances. Faint color variations within the disk suggest subtle differences in stellar populations or dust content across its structure, but the overall impression is that of a fairly homogenous system.
