The galaxy presents as a singular, largely featureless object. Its morphology appears predominantly smooth, with a highly concentrated central region. There is no discernable spiral structure or obvious disk-like component. The light profile is generally round. Color gradients suggest a yellow to redder hue toward the core, possibly indicative of an older stellar population or significant dust obscuration within the central region. There are no obvious signs of ongoing major merger activity or tidal disturbances, though a very slight asymmetry cannot be entirely ruled out due to image resolution. The overall appearance suggests a system that is relatively undisturbed.
