The galaxy presents a generally smooth morphology with a slightly elongated, near-elliptical shape. The galaxy's color profile reveals a central concentration of light exhibiting a subtle bluish-white hue, suggesting the presence of a relatively older stellar population and minimal ongoing star formation within the core. The surrounding halo exhibits a redder tint than the core. There are no clear signs of spiral arm structures or significant dust lanes. Subtle irregularities in the outer regions hint at potential minor gravitational disturbances or past interactions. Overall, the galaxy appears to be a relatively quiescent system, nearing the red sequence.
