The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core region exhibits a brighter, more yellow hue, suggesting an older stellar population and potentially a more significant concentration of dust. Extending outwards from the core, the light gradually fades into a less defined halo. This suggests a transition to a region with lower stellar density.

The overall shape is slightly elongated, appearing somewhere between round and cigar-shaped. There is little indication of strong tidal features or any major disturbances. The galaxy is likely in a relatively quiescent state with no prominent ongoing merger activity. The lack of distinct spiral arms or other complex structures further supports this assessment. The galaxy exhibits moderate size and luminosity.
