The galaxy presents as a somewhat elongated, diffuse object, exhibiting a moderate degree of central concentration. A distinct, yellowish-white core region dominates the galaxy's morphology, suggesting a substantial population of older stars or a possible active galactic nucleus. A faint, greenish-blue halo surrounds the central core, hinting at the presence of younger, star-forming regions, or perhaps emission from ionized gas. There is subtle evidence of a disk-like structure, with a deviation from perfect sphericity. No prominent spiral arms or bar features are discernible within the available image resolution. The overall smoothness of the light distribution indicates a well-mixed stellar population or the possibility of past or ongoing merger activity that has disrupted any pre-existing spiral structure. A slight disturbance in the light distribution is visible. The object presents a low star formation rate.
