This galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth and concentrated light distribution. There is minimal evidence of spiral arms or distinct disk-like structures within the observed image. The galaxy's overall shape is moderately elliptical. The light is more concentrated in the core, which appears yellowish in color, suggesting an older stellar population. The galaxy's halo appears slightly bluer than the core, which suggests possible star formation activity. There is no clear indication of any ongoing major merging events or significant tidal disturbances in the image, although the galaxy appears slightly disturbed.
