The galaxy appears to be a luminous, elliptical system exhibiting a smooth morphology. The central region displays a bright, concentrated core that is indicative of an older stellar population. Diffuse light extends outwards from the core in an oval shape, decreasing in intensity with radial distance. The color profile appears relatively uniform across the galaxy, with a slight redder hue, which supports the classification of an early-type galaxy. There is some evidence of a disturbance or interaction with a merging event that may have contributed to its irregular shape.