The galaxy presents as an elliptical or lenticular type, with a generally smooth and centralized light distribution, lacking prominent spiral arms or a distinct disk structure. The galaxy core exhibits a bright, concentrated luminosity. Moving outwards from the center, the light gradually fades, with no strong indications of ongoing star formation.

The overall shape of the galaxy appears round to slightly elliptical. There's a subtle hint of asymmetry or a minor disturbance in its morphology, which could be attributed to a minor gravitational interaction with another galaxy. There isn't an obvious large-scale merger in progress or any major disturbance in morphology.
