The galaxy presents an overall elliptical morphology, exhibiting a smooth and concentrated light profile. The central region displays a bright, yellowish core, suggestive of an older stellar population. This gradually transitions into a less intense, outer disk-like structure with a slightly flattened shape. Patches of redder hues are observed along the equatorial region. This could be indicative of dust lanes or regions of ongoing, albeit limited, star formation. Overall, the galaxy appears to be a relatively evolved system with characteristics somewhere between a spiral and an elliptical, but with its light dominated by older stars and a smooth morphology, it looks closer to an elliptical galaxy.
