The galaxy presents as an elliptical-like morphology, exhibiting a generally smooth light distribution, with only a slight deviation from perfect circularity. The core region displays a more concentrated luminosity profile, gradually decreasing in intensity toward the outer edges. Coloration suggests an evolved stellar population, with a notable absence of distinct blue star-forming regions. There is a subtle asymmetry and possible hint of a disk, though that interpretation remains uncertain. The galaxy does not appear to be undergoing any major merger events, though slight irregularities could be interpreted as minor disturbances or faint tidal features.
