The galaxy appears as a smooth, elongated structure, likely an elliptical or lenticular galaxy viewed at an oblique angle. The central region exhibits a higher concentration of luminosity, gradually fading towards the outer edges, suggesting a concentration of older stellar populations. The galaxy appears primarily yellow-orange in color, indicative of an evolved stellar population, though there may be some subtle blue hints on the outer edges of the disk. There is no clear indication of spiral arm structure or significant dust lanes, and appears undisturbed.
