The galaxy presents as a relatively smooth, elliptical morphology with a high degree of central concentration. There is no discernible spiral arm structure or significant dust lane obscuration visible at this resolution. The color profile indicates a dominant older stellar population, as evidenced by the yellowish-red hue. The galaxy is elongated, but not drastically so, with an axial ratio suggesting it is close to face-on. A faint, diffuse halo may be present, extending beyond the main body of the galaxy. No major tidal disturbances or signs of ongoing mergers are readily apparent in the image. Overall, the galaxy appears to be a quiescent elliptical, consistent with having a small number of stars forming within it.
