The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright yellow-white core, suggestive of an older stellar population. Moving outwards from the core, the light fades gradually. There is a slight elongation to the galaxy's shape, possibly indicating it is more lenticular than purely elliptical. A faint hint of a bluish tinge can be observed at the periphery on the right, possibly indicating a small amount of recent star formation in that region, or possibly dust. There are no obvious signs of any major ongoing merger events or tidal disturbances. Overall, the galaxy appears to be relatively undisturbed.
