The galaxy presents as a relatively smooth, elliptical structure, exhibiting a central bulge that appears bright and concentrated. The light distribution suggests a primarily older stellar population, with a gradient decreasing outwards from the core. There's a subtle elongation evident in its shape. No prominent spiral arms or significant dust lanes are discernible within the resolution of the image. Faint extensions may be present, but the image quality does not allow for a definite statement. There are no signs of major tidal disturbances or ongoing mergers visible. The overall morphology leans towards a quiescent system.
