The galaxy presents as a centrally concentrated, elliptical-like system. Its overall color appears yellowish-white, suggesting an older stellar population. The light distribution is relatively smooth, with no distinct spiral arm features visible. The core region exhibits a brighter, more intensely luminous area, potentially indicative of a bulge or active galactic nucleus. There is a slight elongation of the galaxy along its major axis. The outer regions fade gradually into the background sky, implying a somewhat diffuse halo structure. There does not appear to be any evidence of significant dust lanes or ongoing major merger activity within the visible structure. Faint, minor disturbances may be present in the morphology of the disk.
