This galaxy presents as a disk-shaped object with a high degree of central concentration. The core region exhibits a bright, yellowish-white color suggesting an older stellar population or a significant amount of dust obscuration. The outer regions appear more diffuse, with hints of bluer components indicating more recent star formation, although these are not well-defined. The galaxy displays a relatively smooth overall appearance, lacking distinct spiral arm structures or prominent irregular features. It appears to be an intermediate galaxy, between an elliptical and spiral type. There is also evidence of a very slight disturbance in the galaxy.
