The galaxy presents a lenticular morphology, appearing as a flattened disk oriented nearly edge-on to our line of sight. A prominent central bulge is visible, displaying a smooth, concentrated luminosity profile characterized by a yellowish hue. The disk component exhibits a bluer color, suggestive of ongoing or recent star formation activity. The overall color gradient indicates a possible radial variation in stellar populations, with older, redder stars concentrated in the bulge and younger, bluer starsPopulating the disk. There is a faint, diffuse extension of light emanating from the disk. I find no signs of major mergers or significant tidal disturbances in this image.
