This galaxy exhibits a distinct spiral morphology, with prominent arms emanating from a central bulge. The spiral arms are tightly wound in some regions, while appearing more open and less defined in others. Two main arms are clearly visible. The central bulge appears moderately sized and luminous. There is evidence of a bar-like structure extending through the central region of the galaxy. The disk of the galaxy is not viewed edge-on. The galaxy does not show any obvious signs of major mergers or significant tidal disturbances, appearing relatively undisturbed. The colors suggest active star formation is taking place within the galaxy, particularly in the spiral arms, but overall the colors are dominated by those consistent with an older stellar population.
