The galaxy presents as a relatively smooth, centrally concentrated object with a slight elongation. There's a discernible color gradient, with a yellowish-white core that fades into a bluer halo or outer region. The overall structure indicates minimal disk features and no obvious spiral arms. Evidence suggests the galaxy may be an elliptical or lenticular type, and the smooth appearance is likely a result of a more quiescent star formation history and/or an older stellar population, with the redder center indicating a higher density of older, cooler stars. There may be a faint dust lane. No active galactic nuclei features or tidal distortions are visible.
