The galaxy presents as a moderately bright, elliptical form, exhibiting a notable central bulge that appears more luminous than the surrounding disk. The disk component appears smooth and featureless, lacking apparent spiral arm structures or prominent dust lanes. Color gradients suggest a concentration of older stellar populations towards the central region, trending to slightly bluer hues in the outer regions of the disk. Overall, the galaxy appears relatively undisturbed, exhibiting a degree of rotational symmetry. There are no obvious signs of recent merger activity or tidal interactions.
