The galaxy presents as a relatively smooth, elliptical structure. Its overall color appears to be a yellowish-orange, suggesting a population of older stars. The galaxy's shape is elongated, with the ratio of its major to minor axis appearing to be approximately 2:1, indicating a significant degree of ellipticity. The light is concentrated toward the center, with a gradual decrease in surface brightness towards the outer edges. There is no clear evidence of spiral arms or other distinct features such as dust lanes or bright knots of star formation. No apparent signs of ongoing or recent major merger activity can be detected.
