The galaxy presents as a single, relatively smooth, and concentrated object. It appears generally elliptical, with a high degree of central concentration that fades into a diffuse halo, though this could be affected by seeing. The light profile suggests an older stellar population, with a color index leaning toward the red end of the spectrum, but still bright in the blue color band. There is no indication of significant disk structures or spiral arms. The galaxy does not show strong signs of recent merging events or tidal disturbances. It may be a relatively quiescent galaxy, undergoing limited star formation.
