This galaxy appears to be a relatively smooth, centrally concentrated system. Its overall shape is elliptical or possibly a lenticular disk. The core displays a higher surface brightness, indicating a concentrated population of stars. The color gradient suggests a bulge with an older stellar population. Fainter, bluer light in the outer regions might imply some ongoing or recent star formation. There is no evidence of strong spiral arm structure or major tidal disturbances, although a slight asymmetry or faint feature cannot be ruled out. Overall, the galaxy presents as a moderately massive, relatively evolved system with a hint of recent star formation activity.
