The galaxy exhibits an elliptical morphology, although a disk component cannot be completely ruled out. It is viewed at a significant inclination relative to our line of sight, and appears to be quite centrally condensed with light. The central region displays a yellowish hue, suggesting an older stellar population. The outer regions become fainter and present a bluer color, possibly indicating ongoing, though mild, star formation within the galaxy's disk. There is no clear indication of spiral arms or a strong bar structure. Minor disturbances may be present but are not pronounced. The overall appearance suggests a relatively evolved galaxy.
