This galaxy presents as a relatively smooth, elliptical-like structure, although it exhibits some deviation from perfect ellipticity. The light profile appears to be centrally concentrated with a bright core that gradually diminishes in intensity towards the outer regions. The color gradient suggests an older stellar population, with a yellowish hue dominating the core, subtly transitioning to slightly bluer tones in the outskirts. There is no clear evidence of spiral arms or significant dust lanes. Subtle irregularities at the edges might indicate minor tidal disturbances or a recent minor merger event but are not prominent. The overall impression is that of a mature galaxy with low star formation activity.
