The galaxy presents as a relatively small, elongated object with a smooth, concentrated central bulge. The disk is viewed at an angle, approaching edge-on, which obscures detailed spiral arm structure if present. There is an apparent lack of prominent dust lanes or regions of intense star formation. The color profile indicates a dominant yellowish-white hue, suggesting a stellar population that is largely evolved, with potentially lower ongoing star formation. The morphology of the galaxy doesn't immediately suggest any major merger events. The relatively smooth appearance supports the idea of a more passively evolving system. 
