The galaxy presents a generally smooth morphology, exhibiting a predominantly elliptical or lenticular form. Its central bulge is noticeably prominent and densely concentrated, displaying a yellowish-orange hue, suggesting an older stellar population. The overall shape is close to circular. A faint, diffuse halo of bluer light surrounds the central region, indicating the presence of some younger, star-forming regions, although star formation rates appear low. There is no discernible evidence of spiral arm structures or significant dust lanes within the image. There are no other visible galaxies nearby that indicate it is merging or disturbed.
