This galaxy presents a smooth, elliptical morphology with a central bulge that appears largely spheroidal. The light distribution suggests an evolved stellar population, with a dominant yellow-red hue in the core region indicating older stars. A slight elongation is visible along the horizontal axis. No distinct spiral arms or dust lanes are discernible. The outer regions of the galaxy fade gradually, suggesting a lack of significant ongoing star formation. There's a subtle color gradient, moving from the yellow-red core to slightly bluer hues in the extended halo, possibly indicating a younger stellar population is present in the outskirts, but the galaxy appears quiescent overall. There is no evidence of recent major mergers or tidal disturbances.
