The galaxy presents as an elongated structure with an apparent smooth morphology. Its light is more concentrated at the center, fading towards the edges, suggesting a centrally concentrated distribution of stars. The color gradient shifts from a yellow hue in the central regions to a slightly redder hue in the outer parts of the galaxy. Its shape implies that it might be an early-type spiral galaxy. Its disk may be viewed from a tilted angle. There is no obvious evidence of active star formation, based on a lack of bright blue regions. The galaxy appears to be isolated, with no signs of a recent major merger.
