The galaxy appears as a centrally concentrated object with a generally smooth morphology. There is a prominent, bright central bulge exhibiting a yellowish-white hue, suggesting an older stellar population. Surrounding the central bulge is a fainter, more diffuse disk-like structure. The outer regions of this structure display a faint bluish tint. This bluish coloration may indicate the presence of more recent star formation activity within the galaxy. No distinct spiral arms or prominent dust lanes are readily apparent in the image. The overall structure appears relatively undisturbed, with no signs of major tidal features or ongoing mergers.
