The galaxy appears as a somewhat diffuse, yellowish-orange object. It exhibits a generally smooth morphology, lacking distinct spiral arms or a prominent bar. The central region displays a higher concentration of light, suggesting the presence of a galactic bulge. There is a very slight elongation visible, with no obvious signs of strong tidal interactions or major disturbances, though there is a suggestion of a very small merger in progress, or an artifact. The overall color indicates an older stellar population, with fewer hot, young stars contributing to the visible light. Given the smooth appearance and color, this galaxy might be classified as an elliptical or lenticular galaxy. However, the slight disk-like appearance would suggest it would likely be a lenticular galaxy. The lack of substantial blue color indicates a relatively low rate of star formation.
