The galaxy presents as a fairly smooth, centrally concentrated system, appearing elliptical in shape. The core region exhibits a bright, yellowish hue, suggesting an older stellar population dominates the central bulge. Moving outward from the core, the light gradually diminishes, with a slightly bluer color suggesting the presence of at least some younger stars. The disk appears relatively featureless, with a gradual fading into the background sky. There is no strong evidence of spiral arms, large dust lanes, or other distinct morphological features. Based on the apparent shape and smooth light distribution, it is likely a fairly massive system.
