The galaxy presents as a relatively smooth, centrally concentrated system. The core region exhibits a bright, yellowish-orange hue, suggesting an older stellar population. The overall shape appears largely circular, with a slight deviation towards a more elliptical form. Fainter, diffuse light extends outwards from the core. There is some indication of possible faint, diffuse spiral arms or irregular features in the outer regions of the disk, but these are not particularly well-defined. The galaxy does not appear to be undergoing any major merger events, although there is a hint of asymmetry or minor disturbance in the outer regions. The galaxy's color transitions from yellowish-orange in the core to a greenish tint in the outer regions. The galaxy is estimated to be of substantial size.
