The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light profile appears to gradually decrease in intensity moving outward from the core. There is little evidence of distinct spiral arm structures or strong irregularities in the overall shape of the galaxy; it seems to be somewhere between a sphere and a disk. The central region exhibits a yellowish hue, potentially indicative of an older stellar population. The outer regions show a hint of bluer colors, which may represent areas of more recent star formation, although the overall star formation rate is probably low. There are no obvious signs of tidal tails or significant interactions with nearby galaxies, suggesting the galaxy is relatively undisturbed. The color gradients suggest some variation in stellar populations across the galaxy.
