The galaxy presents as a single, relatively smooth and centrally concentrated object. Its morphology is generally elliptical, with an apparent axis ratio close to unity, indicating a nearly circular projected shape. Color gradients are subtle, with the central region appearing slightly more yellow, suggesting a higher concentration of older stellar populations. There is no obvious evidence of spiral arms or a prominent disk structure. No significant dust lanes or star-forming regions are visible. The galaxy's surface brightness profile appears to decline smoothly from the center outwards, lacking any sharp features or distinct components. There is no obvious evidence of tidal disturbances or ongoing merging activity.
