The galaxy presents an elliptical morphology, exhibiting a smooth, featureless light distribution with no discernible spiral arms or bar structures. Its overall color profile suggests a relatively red population, with a dominant yellowish-orange hue. The galaxy appears to be fairly round in shape, with a slight elongation that could indicate a weak disk component viewed at an angle or tidal interactions. There is a faint, diffuse halo surrounding the brighter central region. No obvious dust lanes or regions of active star formation are visible within the galaxy's main body. Evidence suggests it could be interacting with other galaxies.
