The galaxy appears as a centrally concentrated object with a generally smooth morphology. Its color profile indicates a dominant yellowish hue in the central region, suggesting an older stellar population. The shape approximates a rounded form. There is no apparent evidence of significant spiral arm structure or a pronounced disk component. The overall light distribution suggests a relatively quiescent system, lacking any strong indications of recent major merger events or significant tidal disturbances. Star formation appears to be minimal based on color.
