The galaxy presents as an elliptical morphology with some distortion, suggesting a potential past or ongoing interaction. The galaxy appears elongated, with a visible axial ratio less than unity. The major axis orientation is roughly northwest to southeast.

Color gradients are noticeable within the galaxy. The central region exhibits a yellowish hue, potentially indicating an older stellar population. This yellow region extends through a small arm of the galaxy, suggesting that this is where the bulk of the stellar mass is. Fainter bluer regions are scattered sparsely throughout the galaxy, potentially indicative of more recent star formation.

There appears to be some disturbances that could be minor mergers or tidal forces. The light is very distorted, suggesting that we are viewing this system during an active state.
