The galaxy presents a somewhat amorphous, but generally rounded appearance. The light distribution suggests a smooth profile, with a central concentration of older stars exhibiting a yellowish-orange hue. Surrounding this core, there's a broader, less defined region of bluish-white light, indicating the presence of a younger stellar population and possible ongoing star formation. A faint, irregular extension appears to emanate from the main body of the galaxy. There appears to be some gravitational disturbance or merger activity, possibly in an early stage, as indicated by the clumpy distribution of light in the outer regions and the slight asymmetry of the galaxy's overall form. The galaxy is not perfectly circular; the ellipticity suggests it may be closer to an intermediate type galaxy, but the smooth light profile gives it a lenticular appearance.
