This galaxy exhibits a distinct, elongated morphology. It presents as a smooth, centrally concentrated object with a noticeable lack of prominent spiral arms or other distinct features. The color gradient suggests a redder core region, potentially indicative of an older stellar population, transitioning to slightly bluer hues towards the outer edges. There is no clear evidence of ongoing major mergers or significant tidal disturbances. The galaxy's overall appearance suggests it is likely an elliptical or lenticular galaxy, viewed edge-on or at a high inclination.
