The galaxy presents as a flattened, disk-like structure oriented approximately along its major axis. It exhibits a relatively smooth, centrally concentrated morphology, with the majority of light emanating from the core region. The color profile suggests a potential for some ongoing star formation, with a slightly bluer hue observed towards the outer regions of the disk. There is no clear indication of strong spiral arm structure or prominent dust lanes within the visible extent of the galaxy. It appears undisturbed, and does not present obvious signs of major mergers or interactions. There appears to be some minor irregularity and disturbances in the disk. Overall the light of the galaxy is not particularly bright.
