This galaxy presents as a largely smooth, concentrated luminosity profile. The core region exhibits a strong central brightness, appearing almost stellar-like in its concentration of light. There is a subtle extension of light outwards from the core.

The galaxy's morphology appears to be somewhere between a circular and an elliptical shape; it is neither perfectly round nor highly elongated. There is a very slight hint of a flattened disk.

Color gradients are observed, with the central region appearing bluish-white. The surrounding halo of the galaxy shows a shift towards redder hues, implying a diverse stellar population with older, redder stars contributing more to the outer regions.

There is little to no evidence of strong tidal features, major disturbances, or ongoing merger activity in this image, but there is some potential for a minor disturbance in the galaxy. The galaxy also shows no signs of spiral arms or other significant morphological features.
