The galaxy presents a relatively smooth morphology, appearing as a flattened ellipsoid. The galaxy exhibits a noticeable central bulge, appearing brighter and more concentrated than the surrounding disk. The shape of the galaxy tends towards a cigar shape rather than a perfect circle. There is faint evidence of disk features surrounding the bulge, but they do not dominate the appearance, with a relatively low fraction of disk light compared to the bulge. The galaxy appears as a mostly unperturbed system, with no obvious signs of ongoing mergers or major tidal disturbances, although some minor irregularities in its shape cannot be ruled out. The observed colors suggest a mix of stellar populations. The central bulge appears somewhat redder in color compared to the outer disk, potentially indicating an older stellar population, while the disk has a bluer hue, suggesting more recent star formation activity.
