The galaxy presents a generally elliptical morphology. The light profile appears quite smooth, lacking distinct spiral arm structures. There is a color gradient visible; the core region shows a strong yellow hue, suggestive of an older stellar population, while the outer regions are tinged with redder hues. The roundness of the galaxy indicates that it is likely viewed close to face-on. There are no obvious signs of tidal disturbances or ongoing major mergers; the overall structure appears largely undisturbed. There may be a minor irregular feature or possible smaller system interacting in the outskirts of the galaxy, seen with blue light.
