The galaxy presents as a relatively smooth, elliptical form. Its morphology suggests a mature system with a dominant spheroid component. The color profile indicates a concentrated, reddish central region that transitions to a more greenish hue in the outer regions. This may indicate a central concentration of older stellar populations with diminished recent star formation and potentially a greater abundance of ionized gases further out from the core. There may be a very faint, disk-like feature, however, this needs further analysis. There appears to be no indication of any major merger events or significant tidal disturbances, indicating a period of relative quiescence in its recent past.
