The galaxy presents an elliptical morphology, exhibiting a smooth and somewhat diffuse light distribution. There is a slightly elongated shape with a hint of a bar structure. The central region shows a concentration of light, suggesting an aging stellar population and/or the presence of a supermassive black hole.

The galaxy displays a relatively red color in its core with bluer hues as one moves further out from the center, indicative of younger stars in the outer regions. There is a visible perturbation of the structure in the upper region of the galaxy, possibly due to a minor merger event. 

Overall, the galaxy appears to be a relatively evolved system undergoing minor interactions, with evidence of both older and younger stellar populations.
