The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge. Its color suggests an older stellar population, with a dominant yellowish hue. The isophotes appear generally regular and elliptical. There is no strong evidence of prominent spiral arms or significant dust lanes. The light profile shows a smooth gradient from the core outwards, indicating a lack of significant ongoing star formation across the galactic body. Faint blue edges around the galaxy suggest recent star formation may be occurring in the outer disk or halo, though the dominant feature is the smooth, round bulge. The galaxy does not display obvious signs of tidal disturbances or interactions.
