The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. It shows no prominent spiral arms or distinct disk-like features. The galaxy's light profile decreases gradually from the core outwards, suggesting a relatively homogenous stellar population. Its shape is predominantly round. There is no obvious evidence of active galactic nuclei activity or a strong starburst region. No major tidal disturbances or clear signs of recent mergers are discernible; however, there is potentially very faint disturbance. The overall color suggests a population of older stars, with lower recent star formation. Based on these observations, this galaxy is likely a massive early-type galaxy, possibly a quiescent elliptical or lenticular.
