The galaxy presents as a somewhat rounded, centrally concentrated object with a smooth overall appearance. The central region exhibits a yellowish-orange hue, suggesting an older stellar population. This core fades into a surrounding disk-like structure exhibiting a bluer color profile. This suggests the presence of younger, hotter stars and possibly ongoing star formation within this outer region. There is some slight, subtle asymmetry in the distribution of the bluer light in the disk, possibly indicating a minor interaction or internal disturbance. However, the primary structure does not show any clear signs of major merging events or significant tidal disruption.
