This galaxy appears to be a relatively smooth and rounded system. There is evidence of a central bulge, which exhibits a warmer, more reddish hue than the surrounding disc. The disc itself shows a general blue color, which may indicate the presence of some younger stars. Though largely smooth, there may be very faint suggestions of some spiral structure or faint arms. There is no strong evidence of significant ongoing mergers or major disturbances. Overall, the galaxy presents as a relatively relaxed and evolved system.