The galaxy appears to be an elliptical type, exhibiting a predominantly smooth morphology.  It possesses a slightly elongated shape.  There is a central concentration of light, suggesting the presence of a galactic nucleus. The galaxy's light profile seems to gradually decrease with radial distance from the core, lacking any distinct spiral arm features or prominent dust lanes.  There is a subtle hint of disturbance or asymmetry in the galaxy's outer regions, but the galaxy seems mostly relaxed and undisturbed. Overall, it appears to be a relatively mature system.
