The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that is yellowish-white in color, suggesting an older stellar population. Extending outwards from the bulge is a fainter, somewhat diffuse halo, which is more blue in color, possibly indicating the presence of a younger stellar population. The overall shape is elongated and not perfectly circular. There is no apparent disk structure or spiral arms. There is a suggestion of some minor distortion or irregularity in the outer halo, although no major tidal features or signs of a significant ongoing merger are clearly visible. The galaxy appears fairly isolated with no other large nearby galaxies, supporting its classification as a non-merging system.
