The galaxy appears to be a relatively round, well-defined structure. The central region exhibits a concentrated, yellowish-white glow, suggestive of an older stellar population. A fainter, bluish halo surrounds the central region, possibly indicating the presence of younger, bluer stars in a disk-like structure. There are suggestions of faint, disturbed arms within the galaxy. The galaxy's smooth appearance overall, along with the round shape, might indicate that it is in the later stages of its evolution. However, there is evidence of a slight disturbance in the disk, hinting at the possibility of an interaction. The overall color profile suggests ongoing, albeit subdued, star formation activity.
