The galaxy appears to be an elliptical galaxy with a relatively smooth light distribution and a high degree of central concentration. There is a noticeable asymmetry in the light profile, with a slight extension visible on one side, suggesting a possible minor tidal interaction or disturbance. The galaxy's core exhibits a yellow to orange hue, which becomes redder moving outwards, which is characteristic of an older stellar population, with minimal ongoing star formation. A merging event might also explain the presence of a faint, extended halo of light surrounding the core. There is no visible disk structure or spiral arms. The overall shape is largely circular, with a minor deviation from perfect roundness. There may be some dusty structure in the core.
