The galaxy appears to be a relatively bright, isolated system. It exhibits a generally smooth morphology, with a centrally concentrated bulge-like structure. The color of the galaxy is predominantly yellowish-white, suggesting an older stellar population. There is little evidence of spiral arms or significant dust lanes, although faint features surrounding the central region could indicate the presence of a weak disk. The galaxy shows a high degree of circularity in its overall shape, with a slight hint of elongation. No obvious signs of a major merger or significant tidal disturbances are visible, however there is evidence for some minor disturbance. The galaxy is moderately sized.
