The galaxy appears as a somewhat elongated spheroid, exhibiting a smooth, featureless morphology in the available image. The color profile suggests a concentration of older stellar populations, indicated by the reddish-yellow hue, towards the core. There is no obvious presence of spiral arms or a prominent disk structure visible. No indications of tidal tails or significant morphological disturbances are discernible, suggesting the galaxy is relatively isolated, with no signs of recent major merger events. The galaxy exhibits a moderate degree of ellipticity, appearing somewhat flattened, but not extremely so. The image resolution limits a more detailed examination of subtle features, such as faint dust lanes or globular cluster populations, which may be present.
