The galaxy appears as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that fades into a more diffuse halo. There's a slight elongation in its shape, departing from a perfectly circular form. The galaxy's color profile is predominantly yellowish, suggesting an older stellar population. There is little evidence of spiral arms or significant dust lanes. While the galaxy exhibits no obvious signs of a major ongoing merger, a slight asymmetry or minor disturbance cannot be entirely ruled out based on the available image resolution. The overall morphology suggests this galaxy is an evolved system with a low rate of star formation.
