The galaxy presents a largely smooth and centralized morphology. It appears elliptical, exhibiting a radial symmetry with the highest concentration of light toward the galactic center. The core of the galaxy has a yellow hue, potentially indicating an older stellar population. Moving outwards from the center, a transition to redder tones can be observed in the outer regions, further supporting the dominance of older stars. There is little to no evidence of distinct spiral arms or significant dust lanes. The lack of pronounced features suggests a galaxy with a relatively quiescent star formation rate. Any signs of ongoing merger activity or tidal disturbances are minimal. Based on the colour profile, the galaxy is likely massive.
