The galaxy presents as an elliptical or lenticular structure, exhibiting a relatively smooth light distribution. The core region appears more concentrated and exhibits a yellowish hue, potentially indicative of an older stellar population. Extending outwards from the core, the light gradually diffuses into a more indistinct halo. A subtle flattening is observed, suggesting that the galaxy may possess some degree of rotational support, and it is unlikely to be a perfect sphere. There is no obvious dust lane and little evidence of spiral arms. The overall form is consistent with a relatively evolved system undergoing ongoing, albeit low levels of star formation. There are no obvious signs of major tidal disturbances or interaction with other galaxies. 
