The galaxy presents a predominantly smooth, elliptical morphology. Its light distribution is centrally concentrated, displaying a bright, well-defined nucleus. A gradual decrease in luminosity is observed moving outward from the core. There is a slight elongation in shape, but it remains fairly round overall. The galaxy exhibits a yellow-orange color, indicative of an older stellar population. There is little evidence of spiral arms or significant dust lanes. No major disturbances or signs of recent merger activity are apparent from the image.
