The galaxy presents as a disk-shaped structure, viewed at a nearly edge-on orientation. A prominent central bulge is visible, displaying a concentrated luminosity. The surrounding disk shows a smooth texture with a hint of spiral arms, though the image resolution limits a more detailed assessment of these features. The overall color profile indicates a population of older stars within the bulge, with bluer hues suggesting areas of more recent star formation present in the outer regions of the disk. There may be a minor disturbance present in its morphology. The galaxy does not present signs of a major merger event and appears to be in a relatively quiescent state.
