The galaxy presents a generally smooth appearance with a hint of disk structure. Its morphology tends toward a somewhat elliptical shape, with the majority of its light concentrated in a central bulge. There is a subtle elongation, but it does not appear highly elongated. Color gradients suggest a concentration of older stellar populations, with a redder hue. No prominent dust lanes or spiral arm structures are discernible in the image. There is no obvious indication of ongoing major merger activity, but some minor disturbances could possibly be present in its outer regions. Based on the smooth appearance, it is most likely an early-type spiral, or even an elliptical galaxy with traces of a disk.
