The galaxy presents as a relatively smooth, elongated structure. Its light is dominated by a central bulge, which appears yellowish-white in color. Fainter, bluer extensions are observed along the major axis of the galaxy, suggesting the presence of a disk. The lack of well-defined spiral arms or significant dust lanes indicates a disk that is either viewed edge-on or is relatively featureless. The overall morphology suggests a galaxy that has either undergone significant evolution or possesses a stellar population with limited ongoing star formation. There is no evidence of major disturbances or interactions with other galaxies.
