The galaxy presents an overall elongated, lenticular morphology. It exhibits a prominent central bulge that appears relatively smooth and concentrated, suggesting an older stellar population dominating this region. The disk component is viewed nearly edge-on, exhibiting some dust obscuration along its plane. Faint indications of potential tidal disturbances or minor irregularities exist in the outer regions of the disk, however this could be due to image artifacts. There is a presence of faint blueish regions within the disk, indicating the likelihood of more recent star formation activity. The galaxy displays a color gradient, transitioning from the yellower central bulge to somewhat bluer disk regions.
